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 | MACSJ0717.5+3547 | 109.4283 | 37.7329 | 108.583729 | 37.823554 | 105.833167 | 15.353649 | 180.28338253 | 21.07400371 | 90.0014 | 55841.8814699074 | 2011-10-07 21:09:19 | 55844.0440046296 | 2011-10-10 01:03:22 | 806006010 | 100.5473 | 100 | 100.5473 | 100.5553 | 0 | 100.5553 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 93.847 | 93.847 | 186.8279 | 1 | PROCESSED | 57603.4085763889 | 2016-08-03 09:48:21 | 56240 | 2012-11-09 00:00:00 | 55872.2982523148 | 2011-11-07 07:09:29 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060016 | MACSJ0717.5+3547 is a forming hot cluster located at z=0.55. Chandra observation resolved a >20 keV hot component near its center, in addition to the average ICM temperature of 11.6 keV. With the most luminous radio halo observed to date, the cluster is in a moment of major merging event. It is also associated with a stream of galaxies oriented to the south east. We propose a Suzaku observation with an exposure of 100 ks, aiming at; confirming the bright > 20 keV component, the very hot component (e.g. Nakazawa+ 2010) evidencing the strong merger, and obtain temperature map of the dim diffuse X-ray observed to the south east and the south west to resolve the nature of these emission. With these observation, merging orientation and phase in this very hot cluster can be resolved. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | B | KAZUHIRO NAKAZAWA | JAP | 6 | AO6 | OBSERVING THE FORMATION EPOCH OF A HOT CLUSTER : SUZAKU OBSERVATION OF MACSJ0717.5+3547 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806006010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '806006010'
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