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 NGC7582 349.5472 -42.3304 348.858747 -42.603943 331.723267 -34.368393 348.20905034 -65.68466064 49.5845 54221.7937384259 2007-05-01 19:02:59 54222.3176273148 2007-05-02 07:37:23 702052010 23.9412 25 23.9572 23.9412 0 23.9572 2 2 0 2 1 0 0 21.5816 21.5816 45.256 0 PROCESSED 57538.5368402778 2016-05-30 12:53:03 54695 2008-08-17 00:00:00 54228.073275463 2007-05-08 01:45:31 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021332 We propose to perform 4 Suzaku observations of 25 ks each (for a total of 100 ks) of the bright Seyfert 2 galaxy,NGC 7582.The aim of this proposal is to measure the distance of the gas that absorbs the nuclear radiation, by analyzing the pattern of variability of its column density.NGC7582 is the ideal target for this kind of analysis, because it already showed large variations of the column density of the absorber between X-ray observations taken a few years apart.With the present proposal, we intend to probe a wider range of timescales, from a week to about six months, in order to measure the distance of the absorber from the nucleus. This measure is crucial to understand the nature of the absorber in type 2 objects and the validity of the torus paradigm. EXTRAGALACTIC COMPACT SOURCES 7 A MARCO CHIABERGE USA 2 AO2 MEASURING THE DISTANCE OF THE ABSORBER IN NGC 7582 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702052010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '702052010'

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