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
|
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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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