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 NGC 720 OFFSET 28.2673 -13.4983 27.658292 -13.744232 21.049561 -23.414412 172.55217141 -70.17529179 242.404 55560.2543634259 2010-12-30 06:06:17 55565.2502083333 2011-01-04 06:00:18 805069010 223.9663 150 223.9722 223.9663 0 223.9722 2 2 0 2 1 0 0 13.3571 13.3571 28.3639 0 PROCESSED 57600.5655671296 2016-07-31 13:34:25 55994 2012-03-08 00:00:00 55627.1378009259 2011-03-07 03:18:26 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051503 Models of galaxy formation suggest that as many as half the baryons may reside in an extended, hot halo. Detecting such a halo around a disk galaxy is, however, extremely challenging for current instrumentation. We propose instead to measure the baryon content of an isolated, X-ray bright elliptical galaxy (Mvir~6E12Msun), which provides the best opportunity to take a census of the baryons in a normal, galaxy-scale system. Currently little is known about the total baryon content of such objects, which are the likely end points of spiral galaxy merging. Combined with archival data, our offset pointing will enable the gas to be traced to ~0.75R500, comparable to what has been achieved for galaxy groups and clusters. EXTRAGALACTIC DIFFUSE SOURCES 8 C PHILIP HUMPHREY USA 5 AO5 THE BARYON FRACTION OF AN ISOLATED ELLIPTICAL GALAXY XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805069010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '805069010'

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