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 SERSIC 159-03 348.4959 -42.7314 347.802109 -43.003937 330.666566 -34.355163 348.33340728 -64.81387916 47.3295 53851.5323611111 2006-04-26 12:46:36 53853.2668055556 2006-04-28 06:24:12 801093010 67.7843 70 67.8003 67.8003 67.7843 67.7923 2 2 2 2 1 0 0 41.5833 41.5833 149.8278 2 PROCESSED 57533.6210532407 2016-05-25 14:54:19 54400 2007-10-27 00:00:00 53907.8625231482 2006-06-21 20:42:02 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012045 We propose to observe the cluster of galaxies Sersic 159-03 using a total exposure time of 70 ks to investigate the soft excess emission previously detected in the observations with ROSAT and XMM-Newton. The superior redistribution function of Suzaku will allow us to determine whether the O VII line emission detected with XMM-Newton is of local (Galactic) origin or is emitted by the warm-hot intergalactic medium (WHIM) in the vicinity of the cluster. The strong soft emission around this cluster together with the much improved response function of the XIS detectors at low energies make Sersic 159-03 the most promising target to unambiguously detect the WHIM for the first time in emission with Suzaku. EXTRAGALACTIC DIFFUSE SOURCES 8 A JELLE KAASTRA EUR 1 AO1 O VII LINE EMISSION IN SERSIC 159-03 - WHIM OR GALACTIC ORIGIN? XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801093010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '801093010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏