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
1 A2390 328.3984 17.7035 327.804289 17.467151 337.435653 28.529496 73.96308198 -27.80512015 79.9886 54955.5395486111 2009-05-04 12:56:57 54957.6939583333 2009-05-06 16:39:18 804012010 96.4645 90 96.4645 96.473 0 96.4725 2 2 0 2 1 0 0 85.5386 85.5386 186.1119 1 PROCESSED 57546.5371990741 2016-06-07 12:53:34 55343 2010-05-27 00:00:00 54976.1695023148 2009-05-25 04:04:05 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040011 We propose Suzaku observations of two massive clusters with different radio morphologies, A2219 and A2390, to search for extremely hot (~25 keV) thermal gas. Because of the presence of hot regions indicated in X-ray temperature maps as well as extended radio halo emission, they are the best candidates hosting strongly heated gas due to the past mergers. With the Suzaku broad-band spectroscopy, we can examine properties of very hot gas with high accuracy, and also put constraints on non-thermal emission. This study can only be achieved by the Suzaku's excellent sensitivity to spectral observations over the wide band, and will bring us new insights into physics of gas heating in clusters. EXTRAGALACTIC DIFFUSE SOURCES 8 A NAOMI OTA JAP 4 AO4 SEARCH FOR EXTREMELY HOT GAS IN TWO MASSIVE GALAXY CLUSTERS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804012010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '804012010'

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