DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | A2256N | 256.1941 | 78.9961 | 256.949832 | 79.060716 | 101.697267 | 76.992175 | 111.38046428 | 31.59001765 | 219.8042 | 56234.8690625 | 2012-11-03 20:51:27 | 56236.1877083333 | 2012-11-05 04:30:18 | 807024010 | 62.2855 | 60 | 62.2855 | 62.2855 | 0 | 62.2855 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 76.5361 | 76.5361 | 113.9039 | 0 | PROCESSED | 57607.9455555556 | 2016-08-07 22:41:36 | 56630 | 2013-12-04 00:00:00 | 56260.5238657407 | 2012-11-29 12:34:22 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 070058 | We observe outskirts of the famous merging cluster of galaxies A2256 with 4 pointings (60ks for each), and obtain spatial distributions of temperature, electron density, pressure and entropy. In a recent study, the thermal profiles after a merger are thought to be similar to those at cluster formation age. By comparing the spatial distributions of A2256 with those of nearby relaxed clusters, we observationally study the evolution of thermal spatial properties of the ICM in the course of cluster evolution. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | MADOKA KAWAHARADA | JAP | 7 | AO7 | THERMAL EVOLUTION OF THE ICM STUDIED WITH A2256 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807024010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '807024010'
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