Equivalent to clicking the Sheet command on the Format menu, and then clicking Hide on the Sheet submenu. Hides sheets in the active workbook.
Syntax
WORKBOOK.HIDE(sheet_text, very_hidden)
Sheet_text is the name of the sheet to hide. If omitted, the currently selected sheet(s) are hidden.
Very_hidden specifies how the sheet is hidden. If TRUE, then the sheet name does not appear in the Unhide dialog box. After using this argument, use WORKBOOK.UNHIDE to unhide the sheet. If FALSE or omitted, hides the sheet but does not prevent the sheet's name from appearing in the Unhide dialog box.
Remarks
If the structure of the workbook is protected, you cannot hide any sheets in the workbook.
You cannot hide the last visible sheet in a workbook.
To hide Sheet1:Sheet10, select them first with the WORKBOOK.SELECT function. You can also place the sheets in an array first, as in {"Sheet1", "Sheet2", "Sheet3",...}.
Return to index


The Tea Planter’s Wife by Dinah Jefferies
Nineteen-year-old Gwendolyn Hooper is newly married to a rich and charming widower, eager to join him on his tea plantation, and determined to be the perfect wife and mother. But life in 1920s Ceylon is not what Gwen had expected. Left on her own expecting twins Gwen is faced with a difficult decision which leaves her hiding a heartbreaking secret which could destroy her marriage.
The Night Circus: A Novel by Erin Morgenstern
In 1886 a mysterious travelling circus becomes an international sensation. Open only at night, constructed entirely in black & white, Le Cirque des Reves delights all who wander its circular paths. The story of The Night Circus begins with two magicians who both have different ideas on the best way to train an apprentice in the art of magic. They agree to a challenge and decide to pit their trainees against each other in a game that will take years to complete, a challenge that only one of them will survive.
This is one that I think will divide your group. You will either lose yourself in the magical world of the book or throw it aside!
The Buried Giant by Kazuo Ishiguro
Ishiguro presents us with a fantasy vision of post-Roman Britain, complete with mythical figures, dragons, ogres and pixies. Axl and Beatrice set off across a troubled land of mist and rain in the hope of finding a son they have not seen for years. Their journey will reveal to them dark and forgotten corners of their love for one another.
This is very different from Ishiguro’s other books which is an advantage or a disadvantage depending on your point of view.
Exposure by Helen Dunmore
London, November, 1960: the Cold War is at its height. Spy fever fills the newspapers, and the political establishment knows how and where to bury its secrets. When a highly sensitive file goes missing, Simon Callington is accused of passing information to the Soviets, and arrested. His wife, Lily, suspects that his imprisonment is part of a cover-up, and that more powerful men than Simon will do anything to prevent their own downfall. She knows that she too is in danger, and must fight to protect her children. But what she does not realise is that Simon has hidden vital truths about his past, and may be found guilty of another crime that carries with it an even greater penalty.
This is a story about secrets, the power they have over us and the cost of keeping them. Helen Dunmore writes beautifully and there is plenty of tension to keep the story racing along.
The Lemon Table by Julian Barnes
Julian Barnes has always been a book club favourite. Arthur & George is one of the most read book club titles.
This collection brings together eleven stories written over 10 years, 6 of which were originally published in The New Yorker, and the remainder in venues such as Granta and the TLS.
Originally titled Rage and Age, Barnes has said that these stories were intended to counter the notion that life calms down or gets serene in old age. If you have never read Julian Barnes this is a good starting place. The stories are about ageing and death, but Barnes displays his customary wit and imagination.
The Invention of Wings by Sue Monk Kidd
Fictionalised account of the life of real-life 19th century slavery abolitionist Sarah Grimke. The book tells the story of two young women, one an ambitious white young woman, the other a feisty black slave who is determined not to accept her lot in life. I have not read this myself but I have heard excellent reports of it.
The Gustav Sonata by Rose Tremain
It is the tutor who tells the young Gustav that he must try to be more like a coconut - that he needs a hard shell to protect the softness inside. This is what his native Switzerland has perfected - a shell to protect its neutrality, to keep its people safe. But his beloved friend, Anton, doesn’t want to be safe - a gifted pianist, he longs to make his mark on the world outside.
On holiday one summer in Davos, the boys stumble across a remote building. Long ago, it was a TB sanitorium; now it is wrecked and derelict. Here, they play a game of life and death, deciding which of their imaginary patients must burn. It becomes their secret. The Gustav Sonata begins in the 1930s, under the shadow of the Second World War, and follows the boys into maturity, and middle age, where their friendship is tested as never before.
If you have never read anything by Rose Tremain I would strongly urge you to start. There is hardly a wasted word throughout. This is writing of the highest quality.
Everyone Brave is Forgiven by Chris Cleave
A love story bubbles up through the devastation of London and Malta in the Second World War. Everyone Brave is inspired by the lives of the author’s grandfather, who served in Malta, and his grandmother, who drove ambulances during the Blitz. At 440 plus pages it is an ambitious read but well worth the effort.
Go Set A Watchman by Harper Lee
I must be in a minority as I never read To Kill A Mockingbird but I thoroughly enjoyed this one.
The novel is set during the mid-1950s and features many of the characters from To Kill a Mockingbird some 20 years before. Scout (Jean Louise Finch) has returned to Maycomb from New York to visit her father Atticus. She is forced to grapple with issues both personal and political as she tries to understand both her father’s attitude toward society, and her own feelings about the place where she was born and spent her childhood.
Harper Lee writes in a gentle fashion, painting memorable pictures of her characters.  The former was habit, the latter was used to tell time when he could not move his fingers enough to dig in his watch pocket. He had been a big man before age and arthritis reduced him to medium size.”
I loved this one. It makes you think of your own relationship with aged parents. People often overlook Harper Lee’s humour but it is funny too.
The Road To Little Dribbling: more notes from a small island by Bill Bryson
Our only non-fiction choice this time round. If you are hoping for another Notes from a Small Island it is not quite that but there are several inspired moments that remind you nobody does mocking the Brits as well as Bryson. It is also educational as he tells you little known facts about places he visits. There are a few ‘hobbyhorse’ moments I could have done without but it is well worth a read. He doesn’t pull his punches either and there are several places where he won’t be invited to switch on the Christmas lights anytime soon.


|
Guild Wars 2 - Elite Insights
<IP_ADDRESS>+
JSON doc
|
Class representing a player More...
Properties | |
| string | Account [get, set] |
| Account name of the player More... | |
| int | Group [get, set] |
| Group of the player More... | |
| bool | HasCommanderTag [get, set] |
| Indicates if a player has a commander tag More... | |
| string | Profession [get, set] |
| Profession of the player More... | |
| bool | FriendlyNPC [get, set] |
| Indicates that the JsonPlayer is actually a friendly NPC More... | |
| bool | NotInSquad [get, set] |
| Indicates that the JsonPlayer is not actually part of the squad More... | |
| string | GuildID [get, set] |
| Guild id to be used to fetch from the official API More... | |
| IReadOnlyList< string > | Weapons [get, set] |
| Weapons of the player 0-1 are the first land set, 1-2 are the second land set 3-4 are the first aquatic set, 5-6 are the second aquatic set When unknown, 'Unknown' value will appear If 2 handed weapon even indices will have "2Hand" as value More... | |
| IReadOnlyList< IReadOnlyList< int > > | ActiveClones [get, set] |
| Array of int[2] that represents the number of active clones Array[i][0] will be the time, Array[i][1] will be the number of clones present from Array[i][0] to Array[i+1][0] If i corresponds to the last element that means the status did not change for the remainder of the fight Only relevant for clone summoning capable specs. More... | |
| IReadOnlyList< IReadOnlyList< JsonStatistics.JsonDPS > > | DpsTargets [get, set] |
| Array of Total DPS stats Length == # of targets and the length of each sub array is equal to # of phases More... | |
| IReadOnlyList< IReadOnlyList< IReadOnlyList< int > > > | TargetDamage1S [get, set] |
| Array of int representing 1S damage points Length == # of targets and the length of each sub array is equal to # of phases More... | |
| IReadOnlyList< IReadOnlyList< IReadOnlyList< int > > > | TargetPowerDamage1S [get, set] |
| Array of int representing 1S power damage points Length == # of targets and the length of each sub array is equal to # of phases More... | |
| IReadOnlyList< IReadOnlyList< IReadOnlyList< int > > > | TargetConditionDamage1S [get, set] |
| Array of int representing 1S condition damage points Length == # of targets and the length of each sub array is equal to # of phases More... | |
| IReadOnlyList< IReadOnlyList< IReadOnlyList< double > > > | TargetBreakbarDamage1S [get, set] |
| Array of double representing 1S breakbar damage points Length == # of targets and the length of each sub array is equal to # of phases More... | |
| IReadOnlyList< IReadOnlyList< IReadOnlyList< JsonDamageDist > > > | TargetDamageDist [get, set] |
| Per Target Damage distribution array Length == # of targets and the length of each sub array is equal to # of phases More... | |
| IReadOnlyList< IReadOnlyList< JsonStatistics.JsonGameplayStats > > | StatsTargets [get, set] |
| Stats against targets Length == # of targets and the length of each sub array is equal to # of phases More... | |
| IReadOnlyList< JsonStatistics.JsonPlayerSupport > | Support [get, set] |
| Support stats Length == # of phases More... | |
| IReadOnlyList< JsonDamageModifierData > | DamageModifiers [get, set] |
| Damage modifiers against all More... | |
| IReadOnlyList< IReadOnlyList< JsonDamageModifierData > > | DamageModifiersTarget [get, set] |
| Damage modifiers against targets Length == # of targets More... | |
| IReadOnlyList< JsonBuffsUptime > | BuffUptimes [get, set] |
| List of buff status More... | |
| IReadOnlyList< JsonPlayerBuffsGeneration > | SelfBuffs [get, set] |
| List of buff status on self generation Key is "'b' + id" More... | |
| IReadOnlyList< JsonPlayerBuffsGeneration > | GroupBuffs [get, set] |
| List of buff status on group generation More... | |
| IReadOnlyList< JsonPlayerBuffsGeneration > | OffGroupBuffs [get, set] |
| List of buff status on off group generation More... | |
| IReadOnlyList< JsonPlayerBuffsGeneration > | SquadBuffs [get, set] |
| List of buff status on squad generation More... | |
| IReadOnlyList< JsonBuffsUptime > | BuffUptimesActive [get, set] |
| List of buff status on active time More... | |
| IReadOnlyList< JsonPlayerBuffsGeneration > | SelfBuffsActive [get, set] |
| List of buff status on self generation on active time More... | |
| IReadOnlyList< JsonPlayerBuffsGeneration > | GroupBuffsActive [get, set] |
List of buff status on group generation on active time
| |
| IReadOnlyList< JsonPlayerBuffsGeneration > | OffGroupBuffsActive [get, set] |
List of buff status on off group generation on active time
| |
| IReadOnlyList< JsonPlayerBuffsGeneration > | SquadBuffsActive [get, set] |
| List of buff status on squad generation on active time More... | |
| IReadOnlyList< JsonDeathRecap > | DeathRecap [get, set] |
| List of death recaps Length == number of death More... | |
| IReadOnlyList< JsonConsumable > | Consumables [get, set] |
| List of used consumables More... | |
| IReadOnlyList< long > | ActiveTimes [get, set] |
| List of time during which the player was active (not dead and not dc) Length == number of phases More... | |
| EXTJsonPlayerHealingStats | EXTHealingStats [get, set] |
| Healing stats data More... | |
| EXTJsonPlayerBarrierStats | EXTBarrierStats [get, set] |
| Barrier stats data More... | |
| Properties inherited from GW2EIJSON.JsonActor | |
| string | Name [get, set] |
| Name of the actor More... | |
| int | TotalHealth [get, set] |
| Total health of the actor. -1 if information is missing (ex: players) More... | |
| uint | Condition [get, set] |
| Condition damage score More... | |
| uint | Concentration [get, set] |
| Concentration score More... | |
| uint | Healing [get, set] |
| Healing Power score More... | |
| uint | Toughness [get, set] |
| Toughness score More... | |
| uint | HitboxHeight [get, set] |
| Height of the hitbox, please not that the center of the box is at the feet of the agent More... | |
| uint | HitboxWidth [get, set] |
| Width of the hitbox More... | |
| ushort | InstanceID [get, set] |
| ID of the actor in the instance More... | |
| ulong | TeamID [get, set] |
| The team ID of the actor. Mainly useful for WvW logs to differentiate targets from different servers. In PvE logs, the situation is always a simple Friend vs Foe situation. \ If value is equal to 0 then no information regarding TeamID was present for given actor. More... | |
| IReadOnlyList< JsonMinions > | Minions [get, set] |
| List of minions More... | |
| bool | IsFake [get, set] |
| Indicates that the JsonActor does not exist in reality More... | |
| IReadOnlyList< JsonStatistics.JsonDPS > | DpsAll [get, set] |
| Array of Total DPS stats Length == # of phases More... | |
| IReadOnlyList< JsonStatistics.JsonGameplayStatsAll > | StatsAll [get, set] |
| Stats against all Length == # of phases More... | |
| IReadOnlyList< JsonStatistics.JsonDefensesAll > | Defenses [get, set] |
| Defensive stats Length == # of phases More... | |
| IReadOnlyList< IReadOnlyList< JsonDamageDist > > | TotalDamageDist [get, set] |
| Total Damage distribution array Length == # of phases More... | |
| IReadOnlyList< IReadOnlyList< JsonDamageDist > > | TotalDamageTaken [get, set] |
| Damage taken array Length == # of phases More... | |
| IReadOnlyList< JsonRotation > | Rotation [get, set] |
| Rotation data More... | |
| IReadOnlyList< IReadOnlyList< int > > | Damage1S [get, set] |
| Array of int representing 1S damage points Length == # of phases More... | |
| IReadOnlyList< IReadOnlyList< int > > | PowerDamage1S [get, set] |
| Array of int representing 1S power damage points Length == # of phases More... | |
| IReadOnlyList< IReadOnlyList< int > > | ConditionDamage1S [get, set] |
| Array of int representing 1S condition damage points Length == # of phases More... | |
| IReadOnlyList< IReadOnlyList< double > > | BreakbarDamage1S [get, set] |
| Array of double representing 1S breakbar damage points Length == # of phases More... | |
| IReadOnlyList< IReadOnlyList< int > > | ConditionsStates [get, set] |
| Array of int[2] that represents the number of conditions Array[i][0] will be the time, Array[i][1] will be the number of conditions present from Array[i][0] to Array[i+1][0] If i corresponds to the last element that means the status did not change for the remainder of the fight More... | |
| IReadOnlyList< IReadOnlyList< int > > | BoonsStates [get, set] |
| Array of int[2] that represents the number of boons Array[i][0] will be the time, Array[i][1] will be the number of boons present from Array[i][0] to Array[i+1][0] If i corresponds to the last element that means the status did not change for the remainder of the fight More... | |
| IReadOnlyList< IReadOnlyList< int > > | ActiveCombatMinions [get, set] |
| Array of int[2] that represents the number of active combat minions Array[i][0] will be the time, Array[i][1] will be the number of active combat minions present from Array[i][0] to Array[i+1][0] If i corresponds to the last element that means the status did not change for the remainder of the fight More... | |
| IReadOnlyList< IReadOnlyList< double > > | HealthPercents [get, set] |
| Array of double[2] that represents the health status of the actor Array[i][0] will be the time, Array[i][1] will be health % If i corresponds to the last element that means the health did not change for the remainder of the fight More... | |
| IReadOnlyList< IReadOnlyList< double > > | BarrierPercents [get, set] |
| Array of double[2] that represents the barrier status of the actor Array[i][0] will be the time, Array[i][1] will be barrier % If i corresponds to the last element that means the health did not change for the remainder of the fight More... | |
| JsonActorCombatReplayData | CombatReplayData [get, set] |
| Contains combat replay related data More... | |
Class representing a player
|
getset |
Account name of the player
|
getset |
Array of int[2] that represents the number of active clones
Array[i][0] will be the time, Array[i][1] will be the number of clones present from Array[i][0] to Array[i+1][0]
If i corresponds to the last element that means the status did not change for the remainder of the fight
Only relevant for clone summoning capable specs.
|
getset |
List of time during which the player was active (not dead and not dc)
Length == number of phases
|
getset |
List of buff status
|
getset |
List of buff status on active time
|
getset |
List of used consumables
|
getset |
Damage modifiers against all
|
getset |
Damage modifiers against targets
Length == # of targets
|
getset |
List of death recaps
Length == number of death
|
getset |
Array of Total DPS stats
Length == # of targets and the length of each sub array is equal to # of phases
|
getset |
Barrier stats data
|
getset |
Healing stats data
|
getset |
Indicates that the JsonPlayer is actually a friendly NPC
|
getset |
Group of the player
|
getset |
List of buff status on group generation
|
getset |
Guild id to be used to fetch from the official API
|
getset |
Indicates if a player has a commander tag
|
getset |
Indicates that the JsonPlayer is not actually part of the squad
|
getset |
List of buff status on off group generation
|
getset |
Profession of the player
|
getset |
List of buff status on self generation
Key is "'b' + id"
|
getset |
List of buff status on self generation on active time
|
getset |
List of buff status on squad generation
|
getset |
List of buff status on squad generation on active time
|
getset |
Stats against targets
Length == # of targets and the length of each sub array is equal to # of phases
|
getset |
Support stats
Length == # of phases
|
getset |
Array of double representing 1S breakbar damage points
Length == # of targets and the length of each sub array is equal to # of phases
If the duration of the phase in seconds is non integer, the last point of this array will correspond to the last point
ex: duration === 15250ms, the array will have 17 elements [0, 1000,...,15000,15250]
|
getset |
Array of int representing 1S condition damage points
Length == # of targets and the length of each sub array is equal to # of phases
If the duration of the phase in seconds is non integer, the last point of this array will correspond to the last point
ex: duration === 15250ms, the array will have 17 elements [0, 1000,...,15000,15250]
|
getset |
Array of int representing 1S damage points
Length == # of targets and the length of each sub array is equal to # of phases
If the duration of the phase in seconds is non integer, the last point of this array will correspond to the last point
ex: duration === 15250ms, the array will have 17 elements [0, 1000,...,15000,15250]
|
getset |
Per Target Damage distribution array
Length == # of targets and the length of each sub array is equal to # of phases
|
getset |
Array of int representing 1S power damage points
Length == # of targets and the length of each sub array is equal to # of phases
If the duration of the phase in seconds is non integer, the last point of this array will correspond to the last point
ex: duration === 15250ms, the array will have 17 elements [0, 1000,...,15000,15250]
|
getset |
Weapons of the player
0-1 are the first land set, 1-2 are the second land set
3-4 are the first aquatic set, 5-6 are the second aquatic set
When unknown, 'Unknown' value will appear
If 2 handed weapon even indices will have "2Hand" as value


linefinder.select module¶
Used to create an id file to track the IDs of.
@author: Zach Hafen @contact<EMAIL_ADDRESS>@status: Development
-
class
linefinder.select.
IDSampler
(out_dir, tag, n_samples=100000, ignore_child_particles=False, ignore_duplicates=False, reference_snum_for_duplicates=600, p_types=None, snapshot_kwargs=None)[source]¶ Bases:
object
-
choose_particles_to_sample
()[source]¶ Choose which particles to subsample. This is done by subtracting out any IDs that we don’t want to use for some reason (e.g. if we’re ignoring IDs that have duplicates).
- Modifies:
- self.ids_to_sample (np.ndarray) : An array of the IDs to sample. self.child_ids_to_sample (np.ndarray, optional) : An array of the child IDs to sample.
-
choose_sample_inds
()[source]¶ Select the indices of the target IDs to sample.
- Modifies:
- self.sample_inds (np.array of ints) : Indices of the target IDs to sample.
-
copy_and_open_full_ids
()[source]¶ Copy the full id file and save them.
- Modifies:
- self.f (h5py file) : Opens and creates the file.
-
identify_child_particles
()[source]¶ Get the IDs and Child IDs of all particles that have non-zero Child IDs.
Returns: A set of all the IDs and Child IDs that have non-zero Child IDs. Return type: child_particles (set)
-
identify_duplicate_ids
()[source]¶ Get all IDs that have duplicates at the latest snapshot. This draws data from the same sample as the original.
Returns: A set of all IDs that have duplicates at snum_end. Return type: duplicate_ids (set)
-
-
class
linefinder.select.
IDSelector
(out_dir, tag, snum_start, snum_end, snum_step, p_types, snapshot_kwargs, n_processors=1)[source]¶ Bases:
object
-
format_selected_ids
(selected_ids)[source]¶ Format the data back into arrays.
Returns: Array of selected IDs child_ids (np.array, optional) : Array of selected child IDS Return type: ids (np.array)
-
get_selected_ids
(data_filters)[source]¶ Get a set of all ids that match a set of data filters.
Parameters: data_filters (list of dicts) – The data filters to apply. Returns: Set of selected ids. Return type: selected_ids (set)
-
get_selected_ids_jug
(data_filters)[source]¶ Parallel version of self.get_selected_ids(). Requires a lot of memory, because it will have multiple snapshots open at once.
Parameters: data_filters (list of dicts) – The data filters to apply. Returns: Set of selected ids. Return type: selected_ids (set)
-
get_selected_ids_parallel
(data_filters)[source]¶ Parallel version of self.get_selected_ids(). Requires a lot of memory, because it will have multiple snapshots open at once.
Parameters: data_filters (list of dicts) – The data filters to apply. Returns: Set of selected ids. Return type: selected_ids (set)
-
get_selected_ids_snapshot
(args)[source]¶ Get the IDs for a particular snapshot. Formatted this way primarily for parallelization.
Parameters: args (data_filters, kwargs) – Information needed to get the IDs out for a snapshot. Returns: The IDs in a snapshot that fit the required condition. Return type: selected_ids_snapshot (set)
-
-
class
linefinder.select.
SnapshotIDSelector
(**kwargs)[source]¶ Bases:
galaxy_dive.analyze_data.particle_data.ParticleData
-
add_hubble_flow
()¶ Correct for hubble flow movement.
- Modifies:
- self.data[‘V’] : Accounts for hubble flow, relative to origin
-
base_data_shape
¶ Property for simulation redshift.
-
calc_HI_den
()¶ Calculate the HI density in cgs (cm^-3).
-
calc_H_den
()¶ Calculate the H density in cgs (cm^-3). Assume the H fraction is ~0.75
-
calc_abs_phi
(vector='total gas ang momentum')¶ The angle (in degrees) from some vector, but don’t mirror it around 90 degrees (e.g. 135 -> 45 degrees, 180 -> 0 degrees).
-
calc_ang_momentum
()¶ Calculate the angular momentum.
-
calc_classifications
()¶ Get the classification for each particle, using data from the Angles-Alcazar+16 pipeline. Uses classes from the tracked_particle_data_handling.py module.
Parameters (include in data_p) ‘tracked_p_data_dir’ : Directory containing the tracked-particle data. ‘tracked_p_file_tag’ : Identifying tag for the tracked-particle data.
-
calc_enriched_metal_mass
()¶ Calculate the metal mass that comes from enrichment, not counting mass that’s at the metallicity floor. Assumes that the there will always be at least one particle in the simulation that’s at the metallicity floor.
-
calc_inds
()¶ Calculate the indices the data are located at, prior to any masks.
-
calc_metal_mass
()¶
-
calc_mu
()¶ we track this with metal species now, could do better…
-
calc_num_den
()¶ Calculate the number density (it’s just a simple conversion…).
-
calc_phi
(normal_vector='total ang momentum')¶ Calculate the angle (in degrees) from some vector. By default the vector is the total angular momentum.
-
calc_pressure
()¶ Calculate the pressure in units of K/cm^3.
-
calc_radial_distance
()¶ Calculate the distance from the origin for a given particle.
-
calc_radial_velocity
()¶ Calculate the radial velocity.
-
calc_rho_xy
()¶ Calculate impact parameter in the xy-plane.
-
calc_rho_xz
()¶ Calculate impact parameter in the xz-plane.
-
calc_rho_yz
()¶ Calculate impact parameter in the yz-plane.
-
calc_tangential_velocity
()¶ Calculate the radial velocity.
-
calc_temp
(gamma=1.6666666666666667)¶ Calculate the temperature from the internal energy.
-
calc_velocity_magnitude
()¶ Calculate the radial velocity.
-
center_coords
()¶ Change the location of the origin, if the data isn’t already centered.
- Modifies:
- self.data[‘P’] : Shifts the coordinates to the center.
-
center_vel_coords
()¶ Get velocity coordinates to center on the main halo.
- Modifies:
- self.data[‘V’] : Makes all velocities relative to self.vel_origin
-
central_mask
¶ This mask is used when, for example, finding the velocity of the center of mass.
-
dN_halo
¶ Calculate dN_halo/dX/dlog10Mh or dN_halo/dz/dlog10Mh. X is absorption path length (see for example Ribaudo+11)
- time_units: ‘abs_length’- dN_halo/dX/dlog10Mh
- ‘redshift’ - dN_halo/dz/dlog10Mh
- R_vir: None - Default, assumes given.
- ‘BN’ Calculates R_vir from the mass and redshift
-
dist_to_point
(point, units='default')¶ Calculate the distance to a point for all particles.
point : np array that gives the point
-
filter_data
(data_filters)[source]¶ Put the filters on the dataset
Parameters: data_filters (list of dicts) – The data filters to apply.
-
find_duplicate_ids
()¶ Find all the IDs in the particle data set that have duplicates.
Returns: Array of IDs that have duplicates. Return type: duplicate_ids ( np.ndarray )
-
format_ids
(selected_ids)[source]¶ Turns the ids into a set to be passed back.
Parameters: selected_ids (np.array or list of np.arrays) – IDs to format into a set. Returns: IDs as a set. Return type: ids_set (set)
-
get_data
(data_key, sl=None)¶ Get the data from within the class. Only for getting the data. No post-processing or changing the data (putting it in particular units, etc.) The idea is to calculate necessary quantities as the need arises, hence a whole function for getting the data.
Parameters: Returns: Requested data.
Return type: data (np.ndarray)
-
get_distance_to_point
(point)¶ This is not unit tested.
Parameters: point (array-like of shape (3,)) – The point you want to find the distance to for each particle.
-
get_ids
()[source]¶ Returns: IDs for particles that match the filtered requirements. child_ids (optional) : Child IDs for the particles that match the filtered requirements. Return type: ids
-
get_position_data
(data_key)¶ Get position data (assuming the data starts with an ‘R’)
Parameters: data_key (str) – Key in the data dictionary for the key we want to get Returns: Requested data. Return type: data (np.ndarray)
-
get_potential
(point)¶ This is not unit tested.
Parameters: point (array-like of shape (3,)) – The point you want to find the potential at
-
get_processed_data
(data_key, data_method=<object object>, *args, **kwargs)¶ Get post-processed data. (Accounting for fractions, log-space, etc.).
Parameters: Returns: Requested data, including formatting.
Return type: processed_data (np.ndarray)
-
get_selected_data
(*args, **kwargs)¶ Wrapper for getting masked data.
-
get_velocity_data
(data_key)¶ Get position data (assuming the data starts with a ‘V’)
Parameters: data_key (str) – Key in the data dictionary for the key we want to get Returns: Requested data. Return type: data (np.ndarray)
-
halo_data
¶ Halo data used.
-
handle_data_key_error
(data_key)¶ When get_data() fails to data_key in self.data, it passes the data_key to try and generate that data.
Parameters: data_key (str) – Key to try and generate data for - Modifies:
- self.data[data_key] (np.array) : If it finds a function to generate the data, it will do so
-
hubble_z
¶ Property for the hubble function at specified redshift.
-
iterate_over_method
(method_str, iter_arg, iter_values, method_args)¶ Iterate over a specified method, and get the results out.
Parameters: Returns: [ method( **used_args ) for used_args in all_variations_of_used_args ]
Return type: results (list)
-
length_scale
¶ Property for fiducial simulation length scale.
-
mask_data
(*args, **kwargs)¶ Wrapper for masking data.
-
metallicity_scale
¶ Property for fiducial metallicity scale. By default is z_sun However, a more advanced subclass might set this differently, or this might change in the future.
-
r_scale
¶ Property for scale radius.
-
r_vir
¶ Property for virial radius.
-
redshift
¶ Property for simulation redshift.
-
retrieve_data
()¶
-
retrieve_halo_data
()¶
-
select_ids_snapshot
(data_filters)[source]¶ Select the IDs that match specified conditions in a given snapshot.
Parameters: data_filters (list of dicts) – The data filters to apply.
-
shift
(data, data_key)¶ Shift or multiply the data by some amount. Note that this is applied after logarithms are applied.
data : data to be shifted data_key : Data key for the parameters to be shifted Parameters are a subdictionary of self.kwargs ‘data_key’ : What data key the data is shifted for
-
total_ang_momentum
¶ Calculate the total angular momentum vector.
-
v_c
¶ Property for circular velocity.
-
v_com
¶ Property for the velocity of the center of mass.
-
velocity_scale
¶ Property for fiducial simulation velocity scale.
-


Package com.google.android.exoplayer2
Interface LoadControl
-
- All Known Implementing Classes:
DefaultLoadControl
public interface LoadControl
Controls buffering of media.
-
-
Method Summary
All Methods Instance Methods Abstract Methods Modifier and Type Method Description Allocator
getAllocator()
Returns theAllocator
that should be used to obtain media buffer allocations.long
getBackBufferDurationUs()
Returns the duration of media to retain in the buffer prior to the current playback position, for fast backward seeking.void
onPrepared()
Called by the player when prepared with a new source.void
onReleased()
Called by the player when released.void
onStopped()
Called by the player when stopped.void
onTracksSelected(Renderer[] renderers, TrackGroupArray trackGroups, ExoTrackSelection[] trackSelections)
Called by the player when a track selection occurs.boolean
retainBackBufferFromKeyframe()
Returns whether media should be retained from the keyframe before the current playback position minusgetBackBufferDurationUs()
, rather than any sample before or at that position.boolean
shouldContinueLoading(long playbackPositionUs, long bufferedDurationUs, float playbackSpeed)
Called by the player to determine whether it should continue to load the source.boolean
shouldStartPlayback(long bufferedDurationUs, float playbackSpeed, boolean rebuffering, long targetLiveOffsetUs)
Called repeatedly by the player when it's loading the source, has yet to start playback, and has the minimum amount of data necessary for playback to be started.
-
-
-
Method Detail
-
onPrepared
void onPrepared()
Called by the player when prepared with a new source.
-
onTracksSelected
void onTracksSelected(Renderer[] renderers, TrackGroupArray trackGroups, ExoTrackSelection[] trackSelections)
Called by the player when a track selection occurs.- Parameters:
renderers
- The renderers.trackGroups
- TheTrackGroup
s from which the selection was made.trackSelections
- The track selections that were made.
-
onStopped
void onStopped()
Called by the player when stopped.
-
onReleased
void onReleased()
Called by the player when released.
-
getAllocator
Allocator getAllocator()
Returns theAllocator
that should be used to obtain media buffer allocations.
-
getBackBufferDurationUs
long getBackBufferDurationUs()
Returns the duration of media to retain in the buffer prior to the current playback position, for fast backward seeking.Note: If
retainBackBufferFromKeyframe()
is false then seeking in the back-buffer will only be fast if the back-buffer contains a keyframe prior to the seek position.Note: Implementations should return a single value. Dynamic changes to the back-buffer are not currently supported.
- Returns:
- The duration of media to retain in the buffer prior to the current playback position, in microseconds.
-
retainBackBufferFromKeyframe
boolean retainBackBufferFromKeyframe()
Returns whether media should be retained from the keyframe before the current playback position minusgetBackBufferDurationUs()
, rather than any sample before or at that position.Warning: Returning true will cause the back-buffer size to depend on the spacing of keyframes in the media being played. Returning true is not recommended unless you control the media and are comfortable with the back-buffer size exceeding
getBackBufferDurationUs()
by as much as the maximum duration between adjacent keyframes in the media.Note: Implementations should return a single value. Dynamic changes to the back-buffer are not currently supported.
- Returns:
- Whether media should be retained from the keyframe before the current playback position
minus
getBackBufferDurationUs()
, rather than any sample before or at that position.
-
shouldContinueLoading
boolean shouldContinueLoading(long playbackPositionUs, long bufferedDurationUs, float playbackSpeed)
Called by the player to determine whether it should continue to load the source.- Parameters:
playbackPositionUs
- The current playback position in microseconds, relative to the start of theperiod
that will continue to be loaded if this method returnstrue
. If playback of this period has not yet started, the value will be negative and equal in magnitude to the duration of any media in previous periods still to be played.bufferedDurationUs
- The duration of media that's currently buffered.playbackSpeed
- The current factor by which playback is sped up.- Returns:
- Whether the loading should continue.
-
shouldStartPlayback
boolean shouldStartPlayback(long bufferedDurationUs, float playbackSpeed, boolean rebuffering, long targetLiveOffsetUs)
Called repeatedly by the player when it's loading the source, has yet to start playback, and has the minimum amount of data necessary for playback to be started. The value returned determines whether playback is actually started. The load control may opt to returnfalse
until some condition has been met (e.g. a certain amount of media is buffered).- Parameters:
bufferedDurationUs
- The duration of media that's currently buffered.playbackSpeed
- The current factor by which playback is sped up.rebuffering
- Whether the player is rebuffering. A rebuffer is defined to be caused by buffer depletion rather than a user action. Hence this parameter is false during initial buffering and when buffering as a result of a seek operation.targetLiveOffsetUs
- The desired playback position offset to the live edge in microseconds, orC.TIME_UNSET
if the media is not a live stream or no offset is configured.- Returns:
- Whether playback should be allowed to start or resume.
-
-


Our pizza is made to order, every pizza is unique so you can create your own personal pizza as you like. We are proudly present our freshly made pizza and hand selected from our local produce to you!


{{ name }} has been successfully archivedYour group has now been archived straight away. This means it has been unpublished and that people will not be able to view it on the website. Any events of your group has been published have also been archived Archiving the group means that you will be able republish it at any time in the future. Thank you, Stockport Council |


Dues and Member Equity Billing
{% if accounts %}| Account | Billable Members | Current Member Equity | AMOUNT TO BILL |
|---|---|---|---|
| {{ account }} | {{ account.billable_member_count }} | {{ account.deposit }} | {{ account.potential_bill }} |
| Totals: | {{ total_billable_members }} | {{ total_deposits }} | {{ total_potential_bills }} |
{% endif %}


Welcome
Welcome to NCCUCS Software Engineering Course 2014. Hosted by Dr. Kung Chen @NCCU. The course covers
- Software Engineering
- Agile Project Management and Software Development
- Free and Opensource Software Development
Teams
- Teaching team - github
- [Team 2] CiKachu - github
- [Team 3] DoraBemon - github
- [Team 4] l4d - github
- [Team 5] NCCUCS-SE-5 - github
- [Team 6] NCCUSE6 - github
Week 7 - Quality, Spec, Testing, TDD
Week 6 - Team project presentation
Week 5 - FOSS introduction by legist
Week 4 - g0v introduction by clkao
Week 3 - Version control with git, social coding with github
Workshop 1: Create your team site.

- Create a github organization account for your team.
- Create github organization pages for your team. (Instructions)
- Clone and contribute to your site.
Workshop 2: Add your team site to Students teams
section
You will learn: Fork (clone to github)
, creating branch
, push a branch
, Pull Requests
, remoate (origin and upstream)
, merge
and *rebase*
- Fork this project to your github user/organization.
- Clone the reposotiry from your user/organization.
- Create a branch named
add-my-team
, and switch to the branch. - Edit
index.html
, add the link of your team website to it. - Commit and push your new branch to github.
- Follow the instructions to send a Pull Request
A Full Instruction about how to fork a repo.
Homework: Team work to create a strong, smart and cool robot.
Criterias:
Work with your team to create a strong robot tank to win the game (You will play the blue tank).  Please finish this homework before 3/17.
The game platform is still in development, you may file a bug or suggest a feature or send me Pull Requests to make it better.
Game Rules:
This is not an A.I. nor game design class. But please work with your team to learn the best of git/github and opensource development. There is no rule to win the game. You can modify anything to make your tank stronger and smarter. But if you want to have competitions with the other teams or individuals (which is the coolist part of this homework), please fight in the fair way!


--- layout: default ---
Want to support the group? Why not try one of the following?
1) Share us around! Like a series we do? Share it with others. Write a review. Do whatever you’d like!
2) Why not just comment on a series you enjoy? I always enjoy reading peoples comments.  You don't know if you're doing anything wrong or if people are even enjoying it.
3) Know someone who is willing to help and can translate Korean, Chinese, or Japanese? Why not tell them about us? No previous experience required!
Question or concern not listed here? Contact us at the email below.waterHelloflameHowscansAre@You?gmail.com
You can send any questions to the Contact Email above.


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Overview
Package
Class
Use
Tree
Deprecated
Index
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B
C
D
F
G
H
I
K
L
M
N
O
P
R
S
T
U
W
X
H
hasNextInput()
- Method in class com.galois.hacrypto.req.input.
CopyInput
hasNextInput()
- Method in class com.galois.hacrypto.req.input.
CountInput
hasNextInput()
- Method in class com.galois.hacrypto.req.input.
FixedInput
hasNextInput()
- Method in interface com.galois.hacrypto.req.input.
Input
hasNextInput()
- Method in class com.galois.hacrypto.req.input.
LengthInput
hasNextInput()
- Method in class com.galois.hacrypto.req.input.
RandomInput
hasNextInput()
- Method in class com.galois.hacrypto.req.input.
RngVInput
hasNextInput()
- Method in class com.galois.hacrypto.req.input.
SequenceInput
hasNextLength()
- Method in class com.galois.hacrypto.req.length.
FixedInputLength
hasNextLength()
- Method in interface com.galois.hacrypto.req.length.
InputLength
hasNextLength()
- Method in class com.galois.hacrypto.req.length.
RandomInputLength
hasNextLength()
- Method in class com.galois.hacrypto.req.length.
SequenceLength
hasNextLength()
- Method in class com.galois.hacrypto.req.length.
StepInputLength
hexStringToByteArray(String)
- Static method in class com.galois.hacrypto.test.
Util
from
this stackoverflow post
hexToCUChar(String)
- Static method in class com.galois.hacrypto.test.
CTests
hmacBouncyCastle(int, byte[], byte[])
- Static method in class com.galois.hacrypto.req.output.
Output
Run BouncyCastle HMAC
B
C
D
F
G
H
I
K
L
M
N
O
P
R
S
T
U
W
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Overview
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Class
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Tree
Deprecated
Index
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Frames
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On June 01, 2020, HCB stopped supporting older versions of Internet Explorer. To use this website, please download the latest version of one of the compatible browsers below:
Questions?
Call customer service at 1-888-813-9220 (TTY: 711 for people who are deaf, hard of hearing, or speech disabled.) We’re available Monday through Friday, 8:00 a.m. to 6:00 p.m.


Contact Information
Dr. Nery Sison
Optometric Physician
14700 NE 8TH ST Suite 105
BELLEVUE, WA 98007
We are in the Cascadia Office Park, in the corner of NE 8th and 148th Ave.
Phone:<PHONE_NUMBER>
Fax:<PHONE_NUMBER>
Mon-Thu 8:30am - 5:30pm
Closed for lunch 1:00 - 2:15 pm
Dr. Nery Sison, an alumna from the Bellevue area schools, received her doctorate from Pacific University, College of Optometry in Oregon. Her scholastic emphasis was in contact lenses and behavioral optometry. She graduated with distinction and received a four-year recognition through Beta Sigma Kappa honorary fraternity. We are pleased to welcome you to our practice. Our commitment is not just in meeting your expectations, but in exceeding them - to offer personalized service to you, our valued patient. We know how much your eye health and appearance can mean to the quality of life, we are committed to excellence in servicing your complete eye care needs.
She's a member of the American Optometric Association, it's Contact Lens Section, Washington Association of Optometric Physicians and the National Eye Research Foundation for Orthokeratology.Our full scope practice ranges from contact lenses (soft, gas permeable and CRT) to fashion forward eyewear with the newest technology lenses. Our doctor is certified to treat and detect common conditions such as diabetic retinopathy, eye infections and glaucoma. We look forward to hearing from you.
Dr. Sison has been married to Fred since she graduated in 1985. They are blessed with two children, Daniel and Maria. She and her family enjoy gardening, creative arts and music.


|
You
Don't Have To Be Alone
('N Sync) |
|
I
dont know when we fell apart
The love that we had was like a work of art I used to see heaven in your eyes Now angels are falling from your skies The things we said, were so wrong I havent held you for so long My foolish pride, turns me inside Why did we tell all thoes lies? You can reach for the phone, You dont have to be alone.


2nd quadrant Galactic SNRs
G93.3+6.9
DA 530, 4C(T)55.38.1
- Right Ascension: 20 52 25
- Declination: +55 21
- Size (/arcmin): 27×20
- Type: C?
- Flux density at 1 GHz (/Jy): 9
- Spectral Index: 0.45
Notes: Has been called G93.2+6.7.
- Radio: Shell, with two bright limbs, highly polarised.
- X-ray: Compact central source.
- Distance: HI observations suggest 2.2 kpc.
References:
- Roger & Costain 1976, A&A, 51, 151. DRAO at 1.42 GHz (2'×2.'4: S=6.9 Jy).
ADS
- Haslam et al. 1980, A&A, 92, 57. Effelsberg 100-m at 1.72 GHz (7.'6: S=6.47±0.52 Jy) and 2.7 GHz (4.'4: S=5.64±0.64 Jy), plus review of flux densities.
ADS
- Lalitha et al. 1984, A&A, 131, 196. Effelsberg 100-m at 4.75 GHz (smoothed to 3': S=4.01±0.57 Jy).
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Landecker et al. 1999, ApJ, 527, 866. DRAO at 408 MHz (3.'5×4.'3) and 1.4 GHz (1.'0×1.'2), including polarisation and HI.
ADS
- Foster & Routledge 2003, ApJ, 598, 1005. HI for distance.
ADS
- Kaplan et al. 2004, ApJS, 153, 269. Chandra limits for any compact source.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=10.5±0.7 Jy) and 1420 MHz, including review of flux densities.
ADS
- Jiang et al. 2007, ApJ, 670, 1142. Chandra observations.
ADS
- Bocchino et al. 2008, AdSpR, 41, 407. XMM-Newton observations.
ADS
- Jeong et al. 2012, Ap&SS, 342, 389. CO observations of region.
ADS
Last updated: 28 Apr 2014
G93.7−0.2
CTB 104A, DA 551
- Right Ascension: 21 29 20
- Declination: +50 50
- Size (/arcmin): 80
- Type: S
- Flux density at 1 GHz (/Jy): 65
- Spectral Index: 0.65
Notes: Has been called G93.6−0.2 and G93.7−0.3.
- Radio: Distorted, faint shell.
- Distance: Association with HI features suggests 1.5 kpc.
References:
- Velusamy & Kundu 1974, A&A, 32, 375. NRAO 300-ft at 2.7 GHz (5': S=18.4±1.0 Jy).
ADS
- Mantovani et al. 1982, A&A, 105, 176. Effelsberg 100-m at 1.7 GHz (7.'6: S=53.5±5.0 Jy), plus review of flux densities.
ADS
- Landecker et al. 1985, AJ, 90, 1082. DRAO at 1.4 GHz (smoothed to 2': S=58±6 Jy).
ADS
- Mantovani et al. 1991, A&A, 247, 545. Effelsberg 100-m at 4.75 GHz (smoothed to 3': S=33.5±4.0 Jy), including polarisation, plus review of flux densities.
ADS
- Biggs & Lyne 1996, MNRAS, 282, 691. Pulsar search.
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA search for OH emission.
ADS
- Uyanıker et al. 2002, ApJ, 565, 1022. CGPS 1.4 GHz (49''×54''), including HI, and 408 MHz (2.'8×3.'7).
ADS
- Uyanıker et al. 2003, ApJ, 585, 785. CGPS at 1.4 GHz (1') including polarisation.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=67±6 Jy) and 1420 MHz (~1': S=35±4 Jy), including polarisation and review of flux densities.
ADS
- Gao et al. 2011, A&A, 529, A159. Urumqi 25-m at 5 GHz (9.'5: S=25.0±2.5 Jy), including polarisation and review of flux densities.
ADS
Last updated: 28 Apr 2014
G94.0+1.0
3C434.1
- Right Ascension: 21 24 50
- Declination: +51 53
- Size (/arcmin): 30×25
- Type: S
- Flux density at 1 GHz (/Jy): 13
- Spectral Index: 0.45
- Radio: Incomplete shell, containing HI shell.
- Distance: Association with stellar wind bubble implies 5.2 kpc.
References:
- Willis 1973, A&A, 26, 237. NRAO 300-ft at 2.7 GHz (5': S=6.1±0.8 Jy), and 37-m at 1.7 GHz (S=11±3 Jy).
ADS
- Velusamy & Kundu 1974, A&A, 32, 375. NRAO 300-ft at 2.7 GHz (5': S=5.8±0.4 Jy). Also NRAO 140-ft at 5 GHz (6').
ADS
- Mantovani et al. 1982, A&A, 105, 176. Effelsberg 100-m at 1.7 GHz (7.'6: S=12.0±1.3 Jy), plus review of flux densities.
ADS
- Goss et al. 1984, A&A, 138, 469. WSRT at 610 MHz (smoothed to 100'': S=16±1.7 Jy) and Effelsberg 100-m at 4.75 GHz (2.'4: S=7.2±0.5 Jy).
ADS
- Landecker et al. 1985, AJ, 90, 1082. DRAO at 1.4 GHz (smoothed to 2': S=16±3 Jy).
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Uyanıker et al. 2003, ApJ, 585, 785. CGPS at 1.4 GHz (1') including polarisation.
ADS
- Foster et al. 2004, A&A, 417, 79. DRAO at 1.4 GHz, including HI.
ADS
- Foster 2005, A&A, 441, 1043. CGPS at 408 MHz (2.'8×3.'6) and 1.4 GHz (0.'8×1.'0) for spectral index studies, plus other observations.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=20±2 Jy) and 1420 MHz (~1': S=11.3±1.0 Jy), including review of flux densities.
ADS
- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.'5: S=6.2±0.4 Jy) including polarisation and review of flux densities.
ADS
- Jeong et al. 2012, Ap&SS, 342, 389. CO observations of region.
ADS
- Jeong et al. 2013, ApJ, 770, 105. CO observations of region.
ADS
Last updated: 24 May 2014
G96.0+2.0
- Right Ascension: 21 30 30
- Declination: +53 59
- Size (/arcmin): 26
- Type: S
- Flux density at 1 GHz (/Jy): 0.35
- Spectral Index: 0.6
- Radio: Faint, arc in S, poorly defined in N.
- Distance: Association for HI indicates 4 kpc.
References:
- Kothes et al. 2005, A&A, 444, 871. CGPS at 408 MHz (2.'8×3.'5) and 1.4 GHz (50''×61'') including HI.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=0.42±0.06 Jy) and 1420 MHz (~1': S=0.24±0.02 Jy), including review of flux densities.
ADS
- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.'5: S=0.14±0.02 Jy) including polarisation and review of flux densities.
ADS
Last updated: 24 May 2014
G106.3+2.7
- Right Ascension: 22 27 30
- Declination: +60 50
- Size (/arcmin): 60×24
- Type: C?
- Flux density at 1 GHz (/Jy): 6
- Spectral Index: 0.6
Notes: Incorporates the pulsar wind nebula G106.6+2.9 (the `Boomerang').
- Radio: Faint extended source, which brighter `head' to NE.
- X-ray: Pulsar and wind nebula.
- Point sources: Pulsar.
References:
- Pineault & Joncas 2000, AJ, 120, 3218. DRAO at 408 MHz (3.'5×3.'9: S=10.5±0.3 Jy) and 1.4 GHz (1.'0×1.'2: S=4.9±0.6 Jy), plus HI.
ADS
- Halpern et al. 2001, ApJ, 547, 323. X-ray and radio observations of the `head'.
ADS
- Halpern et al. 2001, ApJ, 552, L125. Pulsar detection.
ADS
- Kothes et al. 2001, ApJ, 560, 236. CGPS at 1.4 GHz, including HI, plus CO and other observations.
ADS
- Ng & Romani 2004, ApJ, 601, 479. Chandra detection of pulsar wind nebula.
ADS
- Kothes et al. 2004, ApJ, 607, 855. HI polarisation absorption.
ADS
- Kothes et al. 2006, ApJ, 638, 225. Effelsberg 100-m at 4.85 (2.'4), 8.35 (1.'4), 10.5 (1.'2) and 32 GHz (0.'45) of pulsar wind nebula, including polarisation.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=8.6±1.0 Jy) and 1420 MHz (~1': S=4.8±0.5 Jy), including polarisation and review of flux densities.
ADS
- Abdo et al. 2007, ApJ, 664, L91. γ-ray observations.
ADS
- Casandjian & Grenier 2008, A&A, 489, 849. γ-ray observations.
ADS
- Acciari et al. 2009, ApJ, 703, L6. γ-ray observations.
ADS
- Gao et al. 2011, A&A, 529, A159. Urumqi 25-m at 5 GHz (9.'5: S=2.0±0.3 Jy), including polarisation and review of flux densities.
ADS
Last updated: 28 Apr 2017
G108.2−0.6
- Right Ascension: 22 53 40
- Declination: +58 50
- Size (/arcmin): 70×54
- Type: S
- Flux density at 1 GHz (/Jy): 8
- Spectral Index: 0.5
- Radio: Faint shell.
- Distance: Possible associated HI structures suggest 3.2 kpc.
References:
- Tian et al. 2007, A&A, 465, 907. DRAO at 408 MHz (2.'8×3.'3: S=11.5±1.2 Jy) and 1.4 GHz (1.'0×1.'2: S=6.6±0.7 Jy) including HI.
ADS
Last updated: 16 Mar 2009
G109.1−1.0
CTB 109
- Right Ascension: 23 01 35
- Declination: +58 53
- Size (/arcmin): 28
- Type: S
- Flux density at 1 GHz (/Jy): 20
- Spectral Index: 0.45
- Radio: Semicircular shell, with the Molecular cloud S152 is to the immediate W.
- Optical: Faint optical filaments.
- X-ray: Semicircular shell, with pulsar at W edge.
- Point sources: Long period X-ray pulsar (magnetar).
- Distance: Various observations imply 3.2 kpc.
References:
- Hughes et al. 1981, ApJ, 246, L127. WSRT at 610 MHz (1': S=40±5 Jy) shows bad CLEAN artefacts.
ADS
- Blair & Kirshner 1981, Nature, 291, 132. Optical spectra.
ADS
- Downes 1983, MNRAS, 203, 695. Effelsberg 100-m at 2.7 GHz (4.'4: S=13.0±1.5 Jy).
ADS
- Sofue et al. 1983, PASJ, 35, 447. NRO 45-m at 10.2 GHz (2.'7).
ADS
- Hughes et al. 1984, ApJ, 283, 147. WSRT at 610 MHz (20'': S=26±3 Jy) 1.4 GHz (10''), DRAO at 1.4 GHz (1'×1.'2: S=16.8±2 Jy) and Algonquin 46-m at 6.5 GHz (4.'5: S=6.7±1 Jy).
ADS
- Braun & Strom 1986, A&AS, 63, 345. WSRT HI observations.
ADS
- Tatematsu et al. 1987, PASJ, 39, 755. NRO 45-m at 10 GHz (2.'7), plus polarisation.
ADS
- Tatematsu et al. 1987, A&A, 184, 279. CO observations of the surroundings (2.'7).
ADS
- Hanson et al. 1988, A&A, 195, 114. EXOSAT of pulsar.
ADS
also see: Hanson et al. 1988, A&A, 207, 204. Erratum.
ADS
- Morini et al. 1988, ApJ, 333, 777. EXOSAT observations.
ADS
- Koyama et al. 1989, PASJ, 41, 461. X-ray observations of pulsar.
ADS
- Coe et al. 1989, MNRAS, 238, 649. IRAS observations of surroundings.
ADS
- Green 1989, MNRAS, 238, 737. OH observations.
ADS
- Tatematsu et al. 1990, ApJ, 351, 157. CO of surroundings, plus X-ray observations.
ADS
- Davies & Coe 1991, MNRAS, 249, 313. Optical and IR observations near pulsar.
ADS
- Fesen & Hurford 1995, AJ, 110, 747. Optical observations.
ADS
- Hurford & Fesen 1995, MNRAS, 277, 549. ROSAT imaging.
ADS
- Rho & Petre 1997, ApJ, 484, 828. ROSAT observations.
ADS
- Parmar et al. 1998, A&A, 330, 175. X-ray observations.
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA search for OH emission.
ADS
- Patel et al. 2001, ApJ, 563, L45. Chandra observations of pulsar.
ADS
- Kothes et al. 2002, ApJ, 576, 169. CGPS at 1.4 GHz (59''×68''), including HI, plus CO observations.
ADS
- Sasaki et al. 2004, ApJ, 617, 322. XMM-Newton observations.
ADS
- Sasaki et al. 2006, ApJ, 642, L149. CO observations of surroundings, plus Chandra observations.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=26±3 Jy) and 1420 MHz (~1': S=17.4±1.2 Jy), including polarisation and review of flux densities.
ADS
- Tian et al. 2010, MNRAS, 404, L1. CGPS for HI absorption.
ADS
- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.'5: S=9.8±0.5 Jy) including polarisation and review of flux densities.
ADS
- Kothes & Foster 2012, ApJ, 746, L4. HI and CO observations of region.
ADS
- Castro et al. 2012, ApJ, 756, 88. Fermi observations.
ADS
- Sasaki et al. 2013, A&A, 552, A45. Chandra observations of NE.
ADS
- Tendulakar et al. 2013, ApJ, 772, 31. Pulsar proper motion study.
ADS
- Vogel et al. 2014, ApJ, 789, 75. NuSTAR observations of pulsar.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
- Nakano et al. 2017, PASJ, 69, 40. Suzaku observations.
ADS
- Sánchez-Cruces et al. 2018, MNRAS, 473, 1705. Optical observations.
ADS
Last updated: 5 Jun 2019
G111.7−2.1
Cassiopeia A, 3C461
- Right Ascension: 23 23 26
- Declination: +58 48
- Size (/arcmin): 5
- Type: S
- Flux density at 1 GHz (/Jy): 2300
- Spectral Index: 0.77
Notes: Presumably the remnant of a late 17th century SN.
- Radio: Bright shell with compact knots and extended plateau of emission; shows secular decline.
- Optical: Fast knots and quasi-stationary flocculli, with many filaments at large radii, and NE `jet'.
- X-ray: Incomplete shell, with hard spectral component.
- Point sources: Central compact X-ray source.
- Distance: Optical expansion gives 3.3 kpc.
References:
- Anderson & Rudnick 1995, ApJ, 441, 307. VLA at 1.4 GHz and 4.8 GHz, for proper motion studies.
ADS
- Kassim et al. 1995, ApJ, 455, L59. VLA at 74 (25'') and 332 MHz (6''), including spectral index comparisons.
ADS
- Anderson & Rudnick 1996, ApJ, 456, 234. VLA for spectral index comparisons.
ADS
- Schwarz et al. 1997, A&AS, 123, 43. WSRT at 1.4 GHz (30'') for HI absorption.
ADS
- O'Sullivan & Green 1999, MNRAS, 303, 575. Flux density changes at 13.5, 15.5 and 16.5 GHz.
ADS
- Agüeros & Green 1999, MNRAS, 305, 957. 151 MHz observations for bulk expansion studies.
ADS
- Gotthelf et al. 2001, ApJ, 552, L39. Chandra observations, showing outer shock.
ADS
- Hwang et al. 2001, ApJ, 560, L175. Chandra observations of Doppler shifted lines.
ADS
- Fesen et al. 2001, AJ, 122, 2644. HST observations.
ADS
- Reynoso & Goss 2002, ApJ, 575, 871. VLA at 5 GHz (6.''0×6.''4) for H2CO absorption studies.
ADS
- Krause et al. 2005, Science, 308, 1604. Spitzer light echoes from surroundings.
ADS
- Ennis et al. 2006, ApJ, 652, 376. Spitzer observations.
ADS
- Kang & Koo 2007, ApJS, 173, 85. SGPS of high velocity HI.
ADS
- Rho et al. 2008, ApJ, 673, 271. Spitzer observations.
ADS
- Rest et al. 2008, ApJ, 681, L81. SN light echo.
ADS
- Krause et al. 2008, Science, 320, 1195. SN light echo spectrum.
ADS
- Helmboldt & Kassim 2009, AJ, 138, 838. Low radio frequency temporal variations.
ADS
- Patnaude & Fesen 2009, ApJ, 697, 535. X-ray proper motions.
ADS
- Barlow et al. 2010, A&A, 518, L138. Herschel observations.
ADS
- Sibthorpe et al. 2010, ApJ, 719, 1553. Akari and sub-mm observations of region.
ADS
- DeLaney et al. 2010, ApJ, 725, 2038. Spitzer and Chandra observations for 3-D structure.
ADS
- Patnaude et al. 2011, ApJ, 729, L28. Chandra observations of fading.
ADS
- Rest et al. 2011, ApJ, 732, 3. SN light echo observations.
ADS
- Fesen et al. 2011, ApJ, 736, 109. HST variability studies.
ADS
- Besel & Krause 2012, A&A, 541, L3. IR light echoes.
ADS
- Rho et al. 2012, ApJ, 747, L6. Akari CO observations.
ADS
- Vogt et al. 2012, ApJ, 750, 155. Spitzer light echoes.
ADS
- Asgekar et al. 2013, A&A, 551, L11. LOFAR of carbon recombination lines.
ADS
- Yang et al. 2013, ApJ, 766, 44. Suzaku spectroscopy.
ADS
- Rutherford et al. 2013, ApJ, 769, 64. Chandra spectroscopy.
ADS
- Milisavljevic & Fesen 2013, ApJ, 772, 134. Optical spectroscopy for 3-D structure.
ADS
- Koo et al. 2013, Science, 342, 1346. IR spectroscopy.
ADS
- DeLaney et al. 2014, ApJ, 785, 7. VLA plus Pie Town at 74 MHz (9'') and comparison with higher frequencies.
ADS
- Arendt et al. 2014, ApJ, 786, 55. Spitzer and Herschel IR observations.
ADS
- Patnaude & Fesen 2014, ApJ, 789, 138. Multi-epoch optical and X-ray observations.
ADS
- Lee et al. 2014, ApJ, 789, 7. Spitzer and CO observations.
ADS
- Vinyaikin 2014, ARep, 58, 626. Time evolution of radio emission.
ADS
- Alarie et al. 2014, MNRAS, 441, 2996. Optical imaging/spectroscopy, including distance from expansion.
ADS
- Grefenstette et al. 2014, Nature, 506, 339. NuSTAR 44Ti observations.
ADS
- Grefenstette et al. 2015, ApJ, 802, 15. NuSTAR observations.
ADS
- Lee et al. 2015, ApJ, 808, 98. WISE, Spitzer and other IR observations.
ADS
- Milisavljevic & Fesen 2015, Science, 347, 526. Near-IR observations.
ADS
- Arnaud et al. 2016, A&A, 586, A134. Planck flux densities at 7 frequencies between 30 and 353 GHz.
ADS
- Kilpatrick et al. 2016, ApJ, 816, 1. CO observations, including broad lines.
ADS
- Fesen & Milisavljevic 2016, ApJ, 818, 17. HST [SIII] and [SII] observations.
ADS
- Koo et al. 2016, ApJ, 821, 20. Spitzer and Herschel flux densities (and comparison with X-ray properties).
ADS
- Wang & Li 2016, ApJ, 825, 102. INTEGRAL observations.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
- Oonk et al. 2017, MNRAS, 465, 1066. LOFAR observations, including H and C lines, 33 to 78 MHz, including 69 MHz (9.''8×11.''2).
ADS
- De Looze et al. 2017, MNRAS, 465, 3309. Spitzer and Herschel observations.
ADS
- Trotter et al. 2017, MNRAS, 469, 1299. Time evolution of radio emission.
ADS
- Grefenstette et al. 2017, ApJ, 834, 19. NuSTAR observations.
ADS
- Sato et al. 2017, ApJ, 836, 225. Multi-epoch Chandra observations.
ADS
- Lee et al. 2017, ApJ, 837, 118. IR observations.
ADS
- Arias et al. 2018, A&A, 612, A110. LOFAR at 30 to 77 MHz (7''×17'').
ADS
- Salas et al. 2018, MNRAS, 475, 2496. LOFAR C recombination lines as 43, 54, 148 and 340 MHz (70'').
ADS
- Sato et al. 2018, ApJ, 853, 46. Chandra and NuSTAR observations.
ADS
- Zhou et al. 2018, ApJ, 865, 6. CO observations.
ADS
- Raymond et al. 2018, ApJ, 866, 128. IR observations.
ADS
- Koo et al. 2018, ApJ, 866, 139. IR observations.
ADS
Last updated: 9 Apr 2019
G113.0+0.2
- Right Ascension: 23 26 50
- Declination: +61 26
- Size (/arcmin): 40×17?
- Type: ?
- Flux density at 1 GHz (/Jy): 4
- Spectral Index: 0.5?
- Radio: Elongated, extent not well defined.
- Point sources: Contains old pulsar.
- Distance: Association for HI indicates 3.1 kpc.
References:
- Kothes et al. 2005, A&A, 444, 871. CGPS at 408 MHz (2.'8×3.'1) and 1.4 GHz (49''×55'') including HI.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3') and 1420 MHz (~1').
ADS
- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.'5: S=1.9±0.5 Jy) including polarisation and review of flux densities.
ADS
Last updated: 28 Apr 2017
G114.3+0.3
- Right Ascension: 23 37 00
- Declination: +61 55
- Size (/arcmin): 90×55
- Type: S
- Flux density at 1 GHz (/Jy): 5.5
- Spectral Index: 0.5
- Radio: Shell, with HII region S165 within the boundary of the remnant.
- Optical: Faint emission in centre and to S.
- Point sources: Pulsar near centre of remnant.
- Distance: Association with HI and other features implies 0.7 kpc.
References:
- Reich & Braunsfurth 1981, A&A, 99, 17. Effelsberg 100-m at 2.7 GHz (4.'4: S=3.6 Jy) and S1.4 GHz=4.4 Jy from 1.4 GHz survey data, plus HI from Maryland–Green Bank survey.
ADS
- Kulkarni et al. 1993, Nature, 362, 135. Pulsar association.
ADS
- Fürst et al. 1993, A&A, 276, 470. Pulsar association.
ADS
- Becker et al. 1996, A&A, 306, 464. ROSAT of pulsar.
ADS
- Fesen et al. 1997, AJ, 113, 767. Optical observations.
ADS
- Reich 2002, in NSPS, p1. Effelsberg 100-m at 2.7 GHz.
ADS
- Mavromatakis et al. 2002, A&A, 383, 1011. Optical observations.
ADS
- Yar-Uyanıker et al. 2004, ApJ, 616, 247. CGPS at 1.4 GHz (49''×55''), including HI (1.'0×1.'1).
ADS
- Tian & Leahy 2006, ChJAA, 6, 543. CGPS at 408 MHz (3.'4×3.'9: S=12.0±6.0 Jy) and 1.4 GHz (1.'0×1.'1: S=9.8±0.8 Jy).
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 1420 MHz (~1': S=5.4±0.8 Jy), including review of flux densities.
ADS
- Gao et al. 2011, A&A, 529, A159. Urumqi 25-m at 5 GHz (9.'5: S=6.9±0.7 Jy), including polarisation and review of flux densities.
ADS
Last updated: 28 Apr 2014
G116.5+1.1
- Right Ascension: 23 53 40
- Declination: +63 15
- Size (/arcmin): 80×60
- Type: S
- Flux density at 1 GHz (/Jy): 10
- Spectral Index: 0.5
- Radio: Distinct shell, with high polarisation.
- Optical: Detected.
- Distance: Association with HI features implies 1.6 kpc.
References:
- Reich & Braunsfurth 1981, A&A, 99, 17. Effelsberg 100-m at 2.7 GHz (4.'4: S=4.7±0.4 Jy) and S1.4 GHz=8.0±0.8 Jy from 1.4 GHz survey data, plus HI from Maryland–Green Bank survey.
ADS
- Fesen et al. 1997, AJ, 113, 767. Optical observations.
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Yar-Uyanıker et al. 2004, ApJ, 616, 247. CGPS at 1.4 GHz (49''×55''), including HI (1.'0×1.'1).
ADS
- Mavromatakis et al. 2005, A&A, 435, 141. Optical observations.
ADS
- Tian & Leahy 2006, ChJAA, 6, 543. CGPS at 408 MHz (3.'4×3.'8: S=15.0±1.5 Jy) and 1.4 GHz (1.'0×1.'1: S=10.6±0. Jy).
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=12.5±1.6 Jy) and 1420 MHz (~1': S=10.3±0.70 Jy), including polarisation and review of flux densities.
ADS
- Gao et al. 2011, A&A, 529, A159. Urumqi 25-m at 5 GHz (9.'5: S=5.7±0.6 Jy), including polarisation and review of flux densities.
ADS
Last updated: 28 Apr 2014
G116.9+0.2
CTB 1
- Right Ascension: 23 59 10
- Declination: +62 26
- Size (/arcmin): 34
- Type: S
- Flux density at 1 GHz (/Jy): 8
- Spectral Index: 0.57
Notes: Has been called G117.3+0.1 and G116.9+0.1.
- Radio: Incomplete shell.
- Optical: Filaments on sky survey.
- X-ray: Centrally brightened, with NE `breakout'.
- Point sources: Pulsar outside rim to E.
- Distance: Association with HI features implies 1.6 kpc.
References:
- Willis 1973, A&A, 26, 237. NRAO 300-ft at 2.7 GHz (5': S=3.9±1.0 Jy), and 37-m at 1.7 GHz (S=5.5±2.0 Jy), plus review of flux densities.
ADS
- van den Bergh et al. 1973, ApJS, 26, 19. Optical observations.
ADS
- Velusamy & Kundu 1974, A&A, 32, 375. NRAO 300-ft at 2.7 GHz (5': S=4.2±0.2 Jy).
ADS
- Angerhofer et al. 1977, A&A, 55, 11. NRAO 140-ft at 5 GHz (6.'8: S=3.0±0.3 Jy).
ADS
- Dickel & Willis 1980, A&A, 85, 55. WSRT at 610 MHz (56''×64'') and 1.4 GHz (22''×25'').
ADS
- Reich & Braunsfurth 1981, A&A, 99, 17. Effelsberg 100-m at 2.7 GHz (4.'4: S=4.8±0.4 Jy) and S1.4 GHz=7.8±0.8 Jy from 1.4 GHz survey data, plus HI from Maryland–Green Bank survey.
ADS
- Lozinskaya 1981, SvAL, 7, 17. Mean optical velocity.
ADS
- Landecker et al. 1982, AJ, 87, 1379. DRAO at 1.42 GHz and HI (2'×2.'3: S=8.3±0.5 Jy), plus review of flux densities.
ADS
also see: Landecker et al. 1983, AJ, 88, 877. Erratum.
ADS
- Fesen et al. 1985, ApJ, 292, 29. Optical spectra.
ADS
- Hailey & Craig 1994, ApJ, 434, 635. Optical spectroscopy.
ADS
- Hailey & Craig 1995, ApJ, 455, L151. ROSAT of nearby pulsar.
ADS
- Fesen et al. 1997, AJ, 113, 767. Optical observations.
ADS
- Craig et al. 1997, ApJ, 488, 307. ROSAT observations.
ADS
- Reich 2002, in NSPS, p1. Effelsberg 100-m at 10.6 GHz (69''), including polarisation.
ADS
- Yar-Uyanıker et al. 2004, ApJ, 616, 247. CGPS at 1.4 GHz (49''×55''), including HI (1.'0×1.'1).
ADS
- Lazendic & Slane 2006, ApJ, 647, 350. X-ray observations.
ADS
- Tian & Leahy 2006, ChJAA, 6, 543. CGPS at 408 MHz (3.'4×3.'8: S=15.0±1.5 Jy) and 1.4 GHz (1.'0×1.'1: S=8.1±0.4 Jy).
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=10.5±0.8 Jy) and 1420 MHz (~1': S=7.0±0.8 Jy), including review of flux densities.
ADS
- Pannuti et al. 2010, AJ, 140, 1787. ASCA and Chandra observations.
ADS
- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.'5: S=3.6±0.4 Jy) including polarisation and review of flux densities.
ADS
- Clark et al. 2017, ApJ, 834, 106. Fermi pulsar detection.
ADS
- Wu et al. 2018, ApJ, 854, 99. Radio detection of pulsar.
ADS
- Zyuzin et al. 2018, MNRAS, 476, 2177. X-ray observations of pulsar.
ADS
- Katsuragawa et al. 2018, PASJ, 70, 110. Suzaku observations.
ADS
Last updated: 11 Jun 2019
G119.5+10.2
CTA 1
- Right Ascension: 00 06 40
- Declination: +72 45
- Size (/arcmin): 90?
- Type: S
- Flux density at 1 GHz (/Jy): 36
- Spectral Index: 0.6
Notes: Has been called G119.5+10.3.
- Radio: Incomplete shell, with `breakout' to NW.
- Optical: Faint diffuse nebulosities.
- X-ray: Centrally brightened.
- Point sources: Central pulsar.
- Distance: Associated HI shell indicates 1.4 kpc.
References:
- Sieber et al. 1979, A&A, 74, 361. Effelsberg 100-m at 2.7 GHz (4.'4: S=23.6±2.8 Jy).
ADS
- Sieber et al. 1981, A&A, 103, 393. Effelsberg 100-m at 2.7 GHz and 1.7 GHz (7.'6: S=31.6±2.5 Jy), and 151 MHz (4': S=62.6±6 Jy).
ADS
- Fesen et al. 1981, ApJ, 247, 148. Optical, including spectra.
ADS
- Fesen et al. 1983, ApJS, 51, 337. Deep [OIII] imagery.
ADS
- Seward 1990, ApJS, 73, 781. Einstein observations.
ADS
- Simonetti 1992, ApJ, 386, 170. VLA observations of background sources for rotation measure studies.
ADS
- Pineault et al. 1993, AJ, 105, 1060. DRAO at 1.4 GHz (1': S=34±4 Jy), plus HI and IRAS.
ADS
- Seward et al. 1995, ApJ, 453, 284. ROSAT observations.
ADS
- Biggs & Lyne 1996, MNRAS, 282, 691. Pulsar search.
ADS
- Slane et al. 1997, ApJ, 485, 221. ASCA and ROSAT observations.
ADS
- Pineault et al. 1997, A&A, 324, 1152. DRAO at 408 MHz (3.'5) and 1.4 GHz (1.'0).
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Brazier et al. 1998, MNRAS, 295, 819. Studies of central, compact γ-ray source.
ADS
- Mavromatakis et al. 2000, A&A, 353, 371. Optical imagery.
ADS
- Roberts et al. 2001, ApJS, 133, 451. ASCA observations.
ADS
- Reich 2002, in NSPS, p1. Effelsberg 100-m at 1.4 GHz (9.'4).
ADS
- Slane et al. 2004, ApJ, 601, 1045. XMM-Newton observations of central source.
ADS
- Halpern et al. 2004, ApJ, 612, 398. Chandra observations of central nebula, plus optical and radio limits for compact source.
ADS
- Casandjian & Grenier 2008, A&A, 489, 849. γ-ray observations.
ADS
- Abdo et al. 2008, Science, 322, 1218. Fermi detection of pulsar.
ADS
- Lin et al. 2010, ApJ, 725, L1. XMM-Newton observations of pulsar.
ADS
- Caraveo et al. 2010, ApJ, 725, L6. XMM-Newton observations of pulsar.
ADS
- Sun et al. 2011, A&A, 535, A64. Urumqi 25-m at 4.8 GHz (9.'5: S=11.6±1.2 Jy) and Effelsberg 100-m at 2.6 GHz (4.'4: S=20.3±2.0 Jy) including polarisation.
ADS
- Lin et al. 2012, MNRAS, 426, 2283. Suzaku observations.
ADS
- Mignani et al. 2013, MNRAS, 430, 1354. Optical limits for pulsar.
ADS
- Aliu et al. 2013, ApJ, 764, 38. γ-ray observations.
ADS
- Li et al. 2016, ApJ, 831, 19. Fermi observations of pulsar.
ADS
- Ackermann et al. 2018, ApJS, 237, 32. Fermi observations.
ADS
Last updated: 9 Apr 2019
G120.1+1.4
Tycho, 3C10, SN1572
- Right Ascension: 00 25 18
- Declination: +64 09
- Size (/arcmin): 8
- Type: S
- Flux density at 1 GHz (/Jy): 50
- Spectral Index: 0.58
Notes: This is the remnant of the Tycho's SN of AD1572.
- Radio: Shell, brightest to the NE.
- Optical: Faint filaments/knots to the NNW, NE and E.
- X-ray: Shell, brighter to the NE.
- Point sources: Faint radio source near centre of the remnant, thought to be extragalactic.
- Distance: HI observations suggest 2.3–3 kpc, optical proper motion and shock velocity gives 2.4 kpc.
References:
- Duin & Strom 1975, A&A, 39, 33. WSRT at 610 MHz (57''×64'') and 5 GHz (7''×8'').
ADS
- Klein et al. 1979, A&A, 76, 120. Effelsberg 100-m at 10.7 GHz (1.'2: S=13.1±0.8 Jy), plus review of flux densities.
ADS
- Strom et al. 1982, MNRAS, 200, 473. WSRT at 1415 MHz (27''×31'') from 1971 and 1979, for expansion.
ADS
- Dickel et al. 1982, ApJ, 257, 145. Comparison of radio, X-ray and optical observations.
ADS
- Reid et al. 1982, ApJ, 261, 485. Einstein observations.
ADS
- Seward et al. 1983, ApJ, 266, 287. Einstein observations.
ADS
- Tan & Gull 1985, MNRAS, 216, 949. Radio at 2.7 GHz (4'') from 1980 and 1983, and One-Mile Telescope at 1.4 GHz (23'') from 1965 and 1980, for expansion.
ADS
- Albinson et al. 1986, MNRAS, 219, 427. HI observations.
ADS
- Green & Gull 1987, MNRAS, 224, 1055. VLA HI absorption observations towards central radio source.
ADS
- Wood et al. 1992, AJ, 103, 1338. VLA at 5 GHz (1.''5) polarisation studies.
ADS
- Vancura et al. 1995, ApJ, 441, 680. X-ray spectra and ROSAT image.
ADS
- Predehl & Schmitt 1995, A&A, 293, 889. ROSAT of dust scattered halo.
ADS
- Schwarz et al. 1995, A&A, 299, 193. WSRT and Effelsberg 100-m at 1.4 GHz (50''), and VLA at 1.4 GHz (13''), for neutral hydrogen studies.
ADS
- Hwang & Gotthelf 1997, ApJ, 475, 665. ASCA observations.
ADS
- Reynoso et al. 1997, ApJ, 491, 816. VLA at 1.4 GHz (1.''4×1.''5) from 1984 and 1994 for expansion studies.
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Reynoso et al. 1999, AJ, 117, 1827. VLA at 1.4 GHz (13''), for HI studies.
ADS
- Katz-Stone et al. 2000, ApJ, 529, 453. VLA at 333 MHz and 1.4 GHz (7.''7×9.''5), for spectral index studies.
ADS
- Ghavamian et al. 2000, ApJ, 535, 266. Optical observations of shock precursors.
ADS
also see: Ghavamian et al. 2017, ApJ, 843, 77. Erratum.
ADS
- Hughes 2000, ApJ, 545, L53. ROSAT X-ray expansion.
ADS
- Decourchelle et al. 2001, A&A, 365, L218. XMM-Newton observations.
ADS
- Ghavamian et al. 2001, ApJ, 547, 995. Optical spectroscopy.
ADS
- Douvion et al. 2001, A&A, 373, 281. ISO observations.
ADS
- Lee et al. 2004, ApJ, 605, L113. Observations of molecular clouds in vicinity.
ADS
- Warren et al. 2005, ApJ, 634, 376. Chandra observations.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=86±5 Jy) and 1420 MHz (~1': S=40.5±1.5 Jy), including polarisation and review of flux densities.
ADS
- Cassam-Chenaï et al. 2007, ApJ, 665, 315. Chandra observations.
ADS
- Rest et al. 2008, ApJ, 681, L81. SN light echo.
ADS
- Krause et al. 2008, Nature, 456, 617. SN light echo spectrum.
ADS
- Hurley-Walker et al. 2009, MNRAS, 396, 365. Radio observations at 14 to 18 GHz.
ADS
- Raymond et al. 2010, ApJ, 712, 901. Hα spectroscopy.
ADS
- Lee et al. 2010, ApJ, 715, L146. Hα observations.
ADS
- Hayato et al. 2010, ApJ, 725, 894. Suzaku observations of expansion.
ADS
- Ishihara et al. 2010, A&A, 521, L61. Akari observations.
ADS
- Tian & Leahy 2011, ApJ, 729, L15. HI and CO observations.
ADS
- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.'5: S=20.0±2.0 Jy) including polarisation and review of flux densities.
ADS
- Giordano et al. 2012, ApJ, 744, L2. Fermi observations.
ADS
- Gomez et al. 2012, MNRAS, 420, 3557. Herschel IR dust observations.
ADS
- Yang et al. 2013, ApJ, 766, 44. Suzaku spectroscopy.
ADS
- Williams et al. 2013, ApJ, 770, 129. Spitzer observations.
ADS
- Yamaguchi et al. 2014, ApJ, 780, 136. Suzaku observations.
ADS
- Wang & Li 2014, ApJ, 789, 123. INTEGRAL observations.
ADS
- Troja et al. 2014, ApJ, 797, L6. Swift observations.
ADS
- Miceli et al. 2015, ApJ, 805, 120. XMM-Newton observations.
ADS
- Lu et al. 2015, ApJ, 805, 142. Chandra observations.
ADS
- Katsuda et al. 2015, ApJ, 808, 49. Suzaku observations.
ADS
- Tran et al. 2015, ApJ, 812, 101. Chandra observations.
ADS
- Lopez et al. 2015, ApJ, 814, 132. NuSTAR observations.
ADS
- Arnaud et al. 2016, A&A, 586, A134. Planck flux densities at 5 frequencies between 30 and 143 GHz.
ADS
- Koo et al. 2016, ApJ, 821, 20. Spitzer and Herschel flux densities (and comparison with X-ray properties).
ADS
- Williams et al. 2016, ApJ, 823, L32. Multi-epoch X-ray and radio observations for expansion.
ADS
- Zhou et al. 2016, ApJ, 826, 34. CO observations.
ADS
- Chen et al. 2017, A&A, 604, A113. CO observations.
ADS
- Yamaguchi et al. 2017, ApJ, 834, 124. Suzaku observations of E rim.
ADS
- Archambault et al. 2017, ApJ, 836, 23. γ-ray observations.
ADS
- Sato & Hughes 2017, ApJ, 840, 112. Chandra and Suzaku observations.
ADS
- Williams et al. 2017, ApJ, 842, 28. Multi-epoch Chandra observations for expansion studies.
ADS
- Knežević et al. 2017, ApJ, 846, 167. Hα observations of NE.
ADS
- Kerzendorf et al. 2018, MNRAS, 479, 5696. HST search for progenitor companion.
ADS
- Vinyaikin et al. 2018, ARep, 62, 130. Time evolution of radio emission.
ADS
Last updated: 9 Apr 2019
G126.2+1.6
- Right Ascension: 01 22 00
- Declination: +64 15
- Size (/arcmin): 70
- Type: S?
- Flux density at 1 GHz (/Jy): 6
- Spectral Index: 0.5
- Radio: Poorly defined shell.
- Optical: Filaments, mostly in W.
References:
- Reich et al. 1979, A&A, 78, L13. Effelsberg 100-m at 1.4 GHz (9': S=6.8±0.7 Jy) and 2.7 GHz (4.'4: S=3.9±0.4 Jy).
ADS
- Blair et al. 1980, ApJ, 242, 592. Optical detection and spectra.
ADS
- Rosado 1982, RMxAA, 5, 127. Optical spectra.
ADS
- Fesen et al. 1983, ApJS, 51, 337. Deep [OIII] imagery.
ADS
- Fürst et al. 1984, A&A, 133, 11. Effelsberg 100-m at 2.7 GHz (4.'4) and 4.8 GHz (2.'6).
ADS
- Joncas et al. 1989, A&A, 219, 303. DRAO at 408 MHz (3.'5×3.'9: S=12±2.5 Jy) and part at 1.4 GHz (1.'0×1.'1), plus review of flux densities.
ADS
- Xilouris et al. 1993, A&A, 270, 393. Optical imaging.
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Reich et al. 2003, A&A, 408, 961. Effelsberg 100-m at 863 MHz (14.'5: S=6.1±1.6 Jy).
ADS
- Boumis et al. 2005, A&A, 443, 175. Optical observations.
ADS
- Tian & Leahy 2006, A&A, 447, 205. CGPS at 408 MHz (3.'4×3.'8: S=9.7±3.9 Jy) and 1.4 GHz (1.'0×1.'1: S=6.7±2.1 Jy), plus other observations for spectral index studies.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=5.7±0.7 Jy) and 1420 MHz (~1': S=6.4±1.1 Jy), including review of flux densities.
ADS
- Sun et al. 2007, A&A, 463, 993. Urumqi 25-m at 5 GHz (9.'5: S=2.6±0.6 Jy), including polarisation.
ADS
also see: Sun et al. 2007, A&A, 469, 1003. Erratum.
ADS
Last updated: 20 Feb 2009
G127.1+0.5
R5
- Right Ascension: 01 28 20
- Declination: +63 10
- Size (/arcmin): 45
- Type: S
- Flux density at 1 GHz (/Jy): 12
- Spectral Index: 0.45
Notes: Has been called G127.3+0.7.
- Radio: Distinct shell, with bright central source.
- Optical: Detected.
- Point sources: Flat radio spectrum (extragalactic) source at centre of remnant.
- Distance: 1.2–1.3 kpc if associated with NGC 559.
References:
- Caswell 1977, MNRAS, 181, 789. Half-Mile Telescope at 1.42 GHz (3.'5×3.'9), plus other observations of central source.
ADS
- Pauls 1977, A&A, 59, L13. Effelsberg 100-m at 1.4 GHz (9': S=8±1 Jy).
ADS
- Salter et al. 1978, A&A, 66, 77. Effelsberg 100-m at 2.7 GHz (4.'4), plus 5 and 8.7 GHz of the central source.
ADS
- Reich et al. 1979, A&A, 78, L13. Effelsberg 100-m at 1.4 GHz (9': S=10.8±1.3 Jy).
ADS
- Pauls et al. 1982, A&A, 112, 120. WSRT at 610 MHz (56''×62'') and HI absorption to the point source with the VLA.
ADS
- Geldzahler & Shaffer 1982, ApJ, 260, L69. Observations of central source.
ADS
- Fürst et al. 1984, A&A, 133, 11. Effelsberg 100-m at 2.7 GHz (4.'4) and 4.8 GHz (2.'6).
ADS
- Goss & van Gorkom 1984, JApA, 5, 425. WSRT HI absorption of central source.
ADS
- Joncas et al. 1989, A&A, 219, 303. DRAO at 408 MHz (3.'5×3.'9: S=17.9±2.0 Jy) and 1.4 GHz (1.'0×1.'13: S=10.1±0.8 Jy), plus review of flux densities.
ADS
- Xilouris et al. 1993, A&A, 270, 393. Optical imaging.
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Reich et al. 2003, A&A, 408, 961. Effelsberg 100-m at 863 MHz (14.'5: S=14.6±0.8 Jy).
ADS
- Kaplan et al. 2004, ApJS, 153, 269. Chandra limits for any compact sources.
ADS
- Leahy & Tian 2006, A&A, 451, 251. CGPS at 408 MHz (3.'4×3.'8: S=17.1±1.7 Jy) and 1.4 GHz (1.'0×1.'2: S=10.0±0.8 Jy).
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=15.9±1.0 Jy) and 1420 MHz (~1': S=9.7±0.6 Jy), including polarisation and review of flux densities.
ADS
- Sun et al. 2007, A&A, 463, 993. Urumqi 25-m at 5 GHz (9.'5: S=6.3±0.7 Jy), including polarisation.
ADS
also see: Sun et al. 2007, A&A, 469, 1003. Erratum.
ADS
- Zhou et al. 2014, ApJ, 791, 109. CO observations.
ADS
Last updated: 5 May 2017
G130.7+3.1
3C58, SN1181
- Right Ascension: 02 05 41
- Declination: +64 49
- Size (/arcmin): 9×5
- Type: F
- Flux density at 1 GHz (/Jy): 33
- Spectral Index: 0.07
Notes: This is the remnant of the SN of AD1181.
- Radio: Filled-centre, highly polarised, with high frequency turnover.
- Optical: Faint filaments.
- X-ray: Centrally brightened, with faint jet.
- Point sources: Central pulsar.
- Distance: HI absorption indicates 2 kpc.
References:
- Green et al. 1975, A&A, 44, 187. Effelsberg 100-m at 15.0 GHz (58'': S=26.7±0.5 Jy).
ADS
- Wilson & Weiler 1976, A&A, 49, 357. WSRT at 610 MHz (58''×64''), 1.4 GHz (24''×27'') and 5 GHz (7''×8'').
ADS
- van den Bergh 1978, ApJ, 220, L9. Optical observations.
ADS
- Becker et al. 1982, ApJ, 255, 557. X-ray observations.
ADS
- Green & Gull 1982, Nature, 299, 606. HI absorption distance.
ADS
- Fesen 1983, ApJ, 270, L53. Optical spectra.
ADS
- Reynolds & Aller 1985, AJ, 90, 2312. VLA at 1.4 GHz (2'), for limits of shell.
ADS
- Davelaar et al. 1986, ApJ, 300, L59. EXOSAT spectrum.
ADS
- Green 1986, MNRAS, 218, 533. 151 MHz observations (1.'2×1.'3: S=36±4 Jy), plus 2.7 GHz (4''), plus Einstein observations for limit on shell.
ADS
- Green 1987, MNRAS, 225, 11P. Flux density increase at 408 MHz.
ADS
- Morsi & Reich 1987, A&AS, 69, 533. Effelsberg 100-m at 32 GHz (26.''5: S=24.2±1.4 Jy).
ADS
- Reynolds & Aller 1988, ApJ, 327, 845. VLA at 1.4 (2.''4) and 4.9 GHz (2.''5).
ADS
- Salter et al. 1989, ApJ, 338, 171. NRAO 12-m at 84.2 GHz (90'': S=15.0±2.0 Jy), plus review of flux densities.
ADS
- Asaoka & Koyama 1990, PASJ, 42, 625. Ginga X-ray spectrum.
ADS
- Green & Scheuer 1992, MNRAS, 258, 833. IRAS upper limits.
ADS
- Roberts et al. 1993, A&A, 274, 427. HI absorption.
ADS
- Wallace et al. 1994, A&A, 286, 565. HI of surroundings.
ADS
- Helfand et al. 1995, ApJ, 453, 741. ROSAT observations.
ADS
- Torii et al. 2000, PASJ, 52, 875. ASCA observations.
ADS
- Bietenholz et al. 2001, ApJ, 560, 772. VLA at 74 MHz (26'': S=33.6 Jy) and 327 MHz (8.''2: S=33.9 Jy), for spectral index and expansion studies.
ADS
- Bocchino et al. 2001, A&A, 369, 1078. XMM-Newton observations.
ADS
- Murray et al. 2002, ApJ, 568, 226. Chandra pulsar detection.
ADS
- Camilo et al. 2002, ApJ, 571, L41. Pulsar detection in radio.
ADS
- Reich 2002, in NSPS, p1. Effelsberg 100-m at 32 GHz (26'') for polarised intensity.
ADS
- Slane et al. 2002, ApJ, 571, L45. Chandra observations.
ADS
- Slane et al. 2004, ApJ, 616, 403. Deep Chandra imaging.
ADS
- Bietenholz 2006, ApJ, 645, 1180. VLA at 1.4 GHz (1.''36) for expansion studies.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=32.2±2.0 Jy) and 1420 MHz (~1': S=31.9±1.0 Jy), including polarisation and review of flux densities.
ADS
- Gotthelf et al. 2007, ApJ, 654, 267. XMM-Newton observations.
ADS
- Slane et al. 2008, ApJ, 676, L33. Spitzer and other IR observations.
ADS
- Fesen et al. 2008, ApJS, 174, 379. Optical observations for proper motion studies.
ADS
- Shearer & Neustroev 2008, MNRAS, 390, 235. Optical observations of pulsar nebula.
ADS
- Shibanov et al. 2008, A&A, 486, 273. Optical observations of pulsar nebula.
ADS
- Abdo et al. 2009, ApJ, 699, L102. Fermi observations of pulsar.
ADS
- Livingstone et al. 2009, ApJ, 706, 1163. Pulsar observations.
ADS
- Hurley-Walker et al. 2009, MNRAS, 396, 365. Radio observations at 14 to 18 GHz.
ADS
- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.'5: S=31.7±3.0 Jy) including polarisation and review of flux densities.
ADS
- Bietenholz et al. 2013, MNRAS, 431, 2590. Proper motion study of pulsar.
ADS
- Kothes et al. 2013, A&A, 560, A18. CGPS HI observations for distance.
ADS
- Aleksić et al. 2014, A&A, 567, L8. γ-ray detection.
ADS
- Arnaud et al. 2016, A&A, 586, A134. Planck flux densities at 7 frequencies between 30 and 353 GHz.
ADS
Last updated: 13 May 2017
G132.7+1.3
HB3
- Right Ascension: 02 17 40
- Declination: +62 45
- Size (/arcmin): 80
- Type: S
- Flux density at 1 GHz (/Jy): 45
- Spectral Index: 0.6
Notes: Has been called G132.4+2.2.
- Radio: Faint shell, adjacent to W3/4/5 complex.
- Optical: Complete, filamentary shell, shock excited spectra.
- X-ray: Partial shell.
- Point sources: Pulsar nearby.
- Distance: Interaction with surroundings gives 2 kpc.
References:
- van den Bergh et al. 1973, ApJS, 26, 19. Optical observations.
ADS
- Velusamy & Kundu 1974, A&A, 32, 375. NRAO 300-ft at 2.7 GHz (5': S=33.8±7.0 Jy).
ADS
- d'Odorico & Sabbadin 1977, A&AS, 28, 439. Optical spectra.
ADS
- Read 1981, MNRAS, 194, 863. Radio at 151 MHz (4.'4) and 1.4 GHz (2') showing HI shell.
ADS
- Lozinskaya 1981, SvAL, 7, 17. Mean optical velocity.
ADS
- Fesen & Gull 1983, PASP, 95, 196. Optical image.
ADS
- Leahy et al. 1985, ApJ, 294, 183. Einstein observations.
ADS
- Landecker et al. 1987, AJ, 94, 111. DRAO at 408 MHz (3.'5×4': S=75±15 Jy), plus review of flux densities.
ADS
- Routledge et al. 1991, A&A, 247, 529. DRAO at 1.4 GHz (1.'0×1.'1) for HI, plus CO observations.
ADS
- Fesen et al. 1995, AJ, 110, 2876. Optical imaging and spectroscopy, DRAO at 408 MHz (3.'5×4') and 1.4 GHz (1.'0×1.'1).
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA detection of compact OH emission.
ADS
- Reich et al. 2003, A&A, 408, 961. Effelsberg 100-m at 863 MHz (14.'5: S=51.5±3.5 Jy).
ADS
- Tian & Leahy 2005, A&A, 436, 187. CGPS at 408 MHz (3.'4×3.'8:) and 1.4 GHz (1.'0×1.'1), for spectral index studies.
ADS
also see: Tian & Leahy 2006, A&A, 451, 991. Erratum.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=61±9 Jy) and 1420 MHz (~1': S=29.4±2.7 Jy), including review of flux densities.
ADS
- Lazendic & Slane 2006, ApJ, 647, 350. X-ray observations.
ADS
- Green 2007, BASI, 35, 77. Review of radio spectrum.
ADS
- Shi et al. 2008, A&A, 487, 601. Urumqi 25-m at 4.8 GHz (9.'5), plus other survey observations for spectral studies.
ADS
- Casandjian & Grenier 2008, A&A, 489, 849. γ-ray observations.
ADS
- Kilpatrick et al. 2016, ApJ, 816, 1. CO observations, including broad lines.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
- Katagiri et al. 2016, ApJ, 818, 114. Fermi observations.
ADS
- Zhou et al. 2016, ApJ, 833, 4. CO observations of region.
ADS
Last updated: 13 May 2017
G150.3+4.5
- Right Ascension: 04 27 00
- Declination: +55 28
- Size (/arcmin): 180×150
- Type: S
- Flux density at 1 GHz (/Jy): ?
- Spectral Index: ?
- Radio: Faint radio shell.
References:
- Gao & Han 2014, A&A, 567, A59. Radio surveys at 1.4, 2.7 and 5 GHz (9.'4, 4.'3, 9.'5).
ADS
- Ackermann et al. 2017, ApJ, 843, 139. Fermi observations.
ADS
- Ackermann et al. 2018, ApJS, 237, 32. Fermi observations.
ADS
Last updated: 10 Apr 2019
G152.4−2.1
- Right Ascension: 04 07 50
- Declination: +49 11
- Size (/arcmin): 100×95
- Type: S
- Flux density at 1 GHz (/Jy): 3.5?
- Spectral Index: 0.7?
- Radio: Bilateral shell.
References:
- Foster et al. 2013, A&A, 549, A107. Effelsberg 100-m at 2.7 GHz, including polarisation, plus various radio survey observations.
ADS
Last updated: 30 Apr 2014
G156.2+5.7
- Right Ascension: 04 58 40
- Declination: +51 50
- Size (/arcmin): 110
- Type: S
- Flux density at 1 GHz (/Jy): 5
- Spectral Index: 0.5
- Radio: Faint shell, brighter in E and W.
- Optical: Filamentary ring and smaller patchy ring.
- X-ray: Faint shell.
- Distance: Optical/X-ray observations imply >1.7 kpc.
References:
- Pfeffermann et al. 1991, A&A, 246, L28. ROSAT detection.
ADS
- Reich et al. 1992, A&A, 256, 214. Effelsberg 100-m at 1.4 (9': S=4.2±1.0 Jy) and 2.7 GHz (4.'3: S=3.0±1.0 Jy), plus HI and IRAS.
ADS
- Yamauchi et al. 1993, PASJ, 45, 795. Hard X-ray observations.
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Yamauchi et al. 1999, PASJ, 51, 13. ASCA observations of some regions.
ADS
- Reich 2002, in NSPS, p1. Effelsberg 100-m at 2.7 GHz, including polarisation.
ADS
- Pannuti & Allen 2004, AdSpR, 33, 434. ASCA and RXTE observations.
ADS
- Kaplan et al. 2006, ApJS, 163, 344. X-ray upper limit on compact sources.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=8.1±1.3 Jy), including review of flux densities.
ADS
- Xu et al. 2007, A&A, 470, 969. Urumqi 25-m at 4.8 GHz (9.'5: S=2.5±0.5 Jy), including polarisation.
ADS
- Gerardy & Fesen 2007, MNRAS, 376, 929. Optical observations.
ADS
- Katsuda et al. 2009, PASJ, 61, S155. Suzaku observations.
ADS
- Uchida et al. 2012, PASJ, 64, 61. Suzaku observations.
ADS
- Katsuda et al. 2016, ApJ, 826, 108. Multi-epoch Hα observations for expansion.
ADS
Last updated: 13 May 2017
G159.6+7.3
- Right Ascension: 05 20 00
- Declination: +50 00
- Size (/arcmin): 240×180?
- Type: S
- Flux density at 1 GHz (/Jy): ?
- Spectral Index: ?
- Radio: Not detected.
- Optical: Large, faint shell.
- X-ray: Possible emission.
References:
- Fesen & Milisavljevic 2010, AJ, 140, 1163. Hα and ROSAT observations
ADS
Last updated: 8 Jun 2019
G160.9+2.6
HB9
- Right Ascension: 05 01 00
- Declination: +46 40
- Size (/arcmin): 140×120
- Type: S
- Flux density at 1 GHz (/Jy): 110
- Spectral Index: 0.64
Notes: Has been called G160.5+2.8 and G160.4+2.8.
- Radio: Large, filamentary shell.
- Optical: Incomplete shell.
- X-ray: Centrally brightened.
- Point sources: Pulsar within boundary of the remnant, plus several nearby compact radio sources.
- Distance: Various observations suggests less than 4 kpc.
References:
- d'Odorico & Sabbadin 1977, A&AS, 28, 439. Optical spectra.
ADS
- Damashek et al. 1978, ApJ, 225, L31. Pulsar.
ADS
- Lozinskaya 1981, SvAL, 7, 17. Mean optical velocity.
ADS
- Dwarakanath et al. 1982, JApA, 3, 207. Radio observations at 34.5 MHz (26'×40': S=750±150 Jy), plus review of flux densities.
ADS
- van Gorkom et al. 1982, MNRAS, 198, 757. WSRT HI absorption to nearby point source.
ADS
- Seaquist & Gilmore 1982, AJ, 87, 378. VLA observations of nearby source.
ADS
- Leahy 1987, ApJ, 322, 917. Einstein observations.
ADS
- Leahy & Roger 1991, AJ, 101, 1033. DRAO at 408 MHz (3.'5×4.'8) and 1.4 GHz (1.'0×1.'4), including HI and discussion of distance.
ADS
- Yamauchi & Koyama 1993, PASJ, 45, 545. Hard X-ray observations.
ADS
- Leahy & Aschenbach 1995, A&A, 293, 853. ROSAT observations.
ADS
- Biggs & Lyne 1996, MNRAS, 282, 691. Pulsar search.
ADS
- Leahy et al. 1998, A&A, 339, 601. 232 MHz (3.'8×5.'2), 151 MHz (4.'2×5.'8) and Effelsberg 100-m at 4.7 GHz (2.'5) for spectral index studies.
ADS
- Roger et al. 1999, A&AS, 137, 7. 22 MHz flux density (S=1130±340 Jy).
ADS
- Reich et al. 2003, A&A, 408, 961. Effelsberg 100-m at 863 MHz (14.'5: S=91±3 Jy).
ADS
- Fürst & Reich 2004, in MIM, p141. Effelsberg 100-m at 1.4 and 2.7 GHz (9.'3), including polarisation.
ADS
- Kaplan et al. 2006, ApJS, 163, 344. X-ray upper limit on compact sources.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=102±7 Jy) and 1420 MHz (~1': S=54.0±2.9 Jy), including polarisation and review of flux densities.
ADS
- Leahy & Tian 2007, A&A, 461, 1013. CGPS at 408 MHz (2.'8×3.'9: S=117.8±5.3 Jy) and 1.4 GHz (58''×80'': S=65.9±3.4 Jy).
ADS
- Gao et al. 2011, A&A, 529, A159. Urumqi 25-m at 5 GHz (9.'5: S=34±3 Jy), including polarisation and review of flux densities.
ADS
- Gosachinskii 2013, AstL, 39, 179. HI observations of region.
ADS
- Araya et al. 2014, MNRAS, 444, 860. Fermi detection.
ADS
Last updated: 8 Jun 2019
G166.0+4.3
VRO 42.05.01
- Right Ascension: 05 26 30
- Declination: +42 56
- Size (/arcmin): 55×35
- Type: S
- Flux density at 1 GHz (/Jy): 7
- Spectral Index: 0.37
- Radio: Two arcs of strikingly different radii.
- Optical: Nearly complete ring.
- X-ray: Predominantly in SW.
- Distance: HI indicates 4.5 kpc.
References:
- van den Bergh et al. 1973, ApJS, 26, 19. Optical observations.
ADS
- Willis 1973, A&A, 26, 237. NRAO 300-ft at 2.7 GHz (5': S=5.2±1.0 Jy).
ADS
- Lozinskaya 1979, AuJPh, 32, 113. Hα interferometry.
ADS
- Landecker et al. 1982, ApJ, 261, L41. DRAO at 1.4 GHz (1.'0×1.'4), plus review of flux densities.
ADS
- Fesen et al. 1983, ApJS, 51, 337. Deep [OIII] imagery.
ADS
- Pineault et al. 1985, A&A, 151, 52. VLA at 1.4 GHz (16''×20'') of part of remnant, and optical observations.
ADS
- Fesen et al. 1985, ApJ, 292, 29. Optical spectra.
ADS
- Braun & Strom 1986, A&AS, 63, 345. WSRT HI Observations.
ADS
- Pineault et al. 1987, ApJ, 315, 580. DRAO and VLA combined at 1.4 GHz (20'').
ADS
- Landecker et al. 1989, MNRAS, 237, 277. DRAO at 1.4 GHz (1.'0×1.'4), including HI.
ADS
- Burrows & Guo 1994, ApJ, 421, L19. ROSAT images and spectra.
ADS
- Biggs & Lyne 1996, MNRAS, 282, 691. Pulsar search.
ADS
- Guo & Burrows 1997, ApJ, 480, L51. ASCA observations.
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Leahy & Tian 2005, A&A, 440, 929. CGPS at 408 MHz (3.'4×5.'0) and 1.4 GHz (1.'0×1.'4), for spectral index studies.
ADS
also see: Tian & Leahy 2006, A&A, 451, 991. Erratum.
ADS
- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=8.1±0.9 Jy) and 1420 MHz (~1': S=5.1±0.4 Jy), including polarisation and review of flux densities.
ADS
- Bocchino et al. 2009, A&A, 498, 139. XMM-Newton observations.
ADS
- Gao et al. 2011, A&A, 529, A159. Urumqi 25-m at 5 GHz (9.'5: S=3.3±0.3 Jy), including polarisation and review of flux densities.
ADS
- Araya 2013, MNRAS, 434, 2202. Fermi observations.
ADS
- Matsumura et al. 2017, PASJ, 69, 30. Suzaku observations.
ADS
Last updated: 9 Apr 2019
G178.2−4.2
- Right Ascension: 05 25 05
- Declination: +28 11
- Size (/arcmin): 72×62
- Type: S
- Flux density at 1 GHz (/Jy): 2
- Spectral Index: 0.5
- Radio: Faint shell, brighter in NE.
References:
- Gao et al. 2011, A&A, 532, A144. Urumqi 25-m at 5 GHz (9.'5: S=1.0±0.1 Jy), plus other observations.
ADS
Last updated: 28 Apr 2017
G179.0+2.6
- Right Ascension: 05 53 40
- Declination: +31 05
- Size (/arcmin): 70
- Type: S?
- Flux density at 1 GHz (/Jy): 7
- Spectral Index: 0.4
- Radio: Thick shell, with background extragalactic sources near centre.
- Optical: Nearly complete shell.
- Point sources: Pulsar near centre.
References:
- Fürst & Reich 1986, A&A, 154, 303. Effelsberg 100-m at 1.4 (9.'4), 2.7 (4.'3) and 4.75 GHz (2.'4).
ADS
- Fürst et al. 1989, A&A, 223, 66. Observations of central, extragalactic source.
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Reich 2002, in NSPS, p1. Effelsberg 100-m at 2.7 GHz.
ADS
- Gao et al. 2011, A&A, 529, A159. Urumqi 25-m at 5 GHz (9.'5: S=3.2±0.3 Jy), including polarisation and review of flux densities.
ADS
- Jeong et al. 2012, Ap&SS, 342, 389. CO observations of region.
ADS
- Pletsch et al. 2013, ApJ, 779, L11. Pulsar detection.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
- How et al. 2018, MNRAS, 478, 1987. Optical observations.
ADS
Last updated: 8 Jun 2019
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Estimate the abundance of cell clones from the distribution of lengths of DNA fragments (as created by sonication, whence ‘sonicLength’). The algorithm in "Estimating abundances of retroviral insertion sites from DNA fragment length data" by Berry CC, Gillet NA, Melamed A, Gormley N, Bangham CR, Bushman FD. Bioinformatics; 2012 Mar 15;28(6):755-62 is implemented. The experimental setting and estimation details are described in detail there. Briefly, integration of new DNA in a host genome (due to retroviral infection or gene therapy) can be tracked using DNA sequencing, potentially allowing characterization of the abundance of individual cell clones bearing distinct integration sites. The locations of integration sites can be determined by fragmenting the host DNA (via sonication or fragmentase), breaking the newly integrated DNA at a known sequence, amplifying the fragments containing both host and integrated DNA, sequencing those amplicons, then mapping the host sequences to positions on the reference genome. The relative number of fragments containing a given position in the host genome estimates the relative abundance of cells hosting the corresponding integration site, but that number is not available and the count of amplicons per fragment varies widely. However, the expected number of distinct fragment lengths is a function of the abundance of cells hosting an integration site at a given position and a certain nuisance parameter. The algorithm implicitly estimates that function to estimate the relative abundance.
| Version: | 1.4.4 |
| Depends: | R (≥ 2.14.0), splines |
| Published: | 2014-08-24 |
| Author: | Charles Berry |
| Maintainer: | Charles Berry <ccberry at ucsd.edu> |
| License: | GPL-2 | GPL-3 [expanded from: GPL (≥ 2)] |
| NeedsCompilation: | no |
| Citation: | sonicLength citation info |
| CRAN checks: | sonicLength results |
| Reference manual: | sonicLength.pdf |
| Vignettes: |
Estimating Abundances with sonicLength |
| Package source: | sonicLength_1.4.4.tar.gz |
| Windows binaries: | r-devel: sonicLength_1.4.4.zip, r-release: sonicLength_1.4.4.zip, r-oldrel: sonicLength_1.4.4.zip |
| OS X binaries: | r-release: sonicLength_1.4.4.tgz, r-oldrel: sonicLength_1.4.4.tgz |
Please use the canonical form https://CRAN.R-project.org/package=sonicLength to link to this page.


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Basic Grid with the use of Slick.Plugins.Resizer
Fixed Dimensions 800x600
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| bufferUntilSubscribed |
fun <T> Observable<T>.bufferUntilSubscribed(): Observable<T>
Returns an Observable that buffers events until subscribed. |
| toFuture |
fun <T> Observable<T>.toFuture(): ListenableFuture<T>
Returns a ListenableFuture bound to the |


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