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 A2142 OFFSET2 239.2185 27.5666 238.702662 27.710117 228.594218 46.67807 44.63617571 49.06945571 260.7114 54358.4806597222 2007-09-15 11:32:09 54360.0627893518 2007-09-17 01:30:25 802031010 57.7187 50 57.7187 57.7187 0 57.7187 1 1 0 1 1 0 0 52.5976 52.5976 136.6318 1 PROCESSED 57539.9791666667 2016-05-31 23:30:00 54751 2008-10-12 00:00:00 54371.4005208333 2007-09-28 09:36:45 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020076 We propose to search for redshifted OVII and OVIII lines from the warm-hot intergalactic medium (WHIM) in a large-scale filament outside of a massive merging cluster of galaxies A2142. This cluster is characterized by prominent cold fronts, elongated X-ray morphology, and Beppo-SAX detection of hard X-ray emission, which all point to a recent merger and the matter density outside should be high. The strong reason why we choose this target is its right redshift (z=0.909), in which XIS sensitivity for redshifted oxygen lines separated from the Galactic lines becomes the highest. We expect 3 times higher sensitivity than our previous attempt for A2218 (Takei et al. in press) where we set 5 times lower upper limit for OVII line intensity than the XMM reported levels in other clusters. EXTRAGALACTIC DIFFUSE SOURCES 8 B TAKAYA OHASHI JAP 2 AO2 WHIM SEARCH AROUND A MASSIVE MERGING CLUSTER OF GALAXIES A2142 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802031010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '802031010'

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