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.
observation_id
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
exposure
awarded_exposure
resolve_exposure
resolve_data_mode
resolve_with_filter_be
resolve_with_filter_fe55
resolve_with_filter_nd
resolve_with_filter_poly
resolve_with_filter_open
resolve_with_filter_undef
is_resolve_gatevalve_closed
is_resolve_mxs1
is_resolve_mxs2
is_resolve_mxs3
is_resolve_mxs4
resolve_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
ql_access_url
ql_image_url
corner1_ra
corner1_dec
corner2_ra
corner2_dec
corner3_ra
corner3_dec
corner4_ra
corner4_dec
corner5_ra
corner5_dec
corner6_ra
corner6_dec
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_dec_b1950
corner5_ra_b1950
corner5_dec_b1950
corner6_ra_b1950
corner6_dec_b1950
corner1_ecliptic_lon
corner1_ecliptic_lat
corner2_ecliptic_lon
corner2_ecliptic_lat
corner3_ecliptic_lon
corner3_ecliptic_lat
corner4_ecliptic_lon
corner4_ecliptic_lat
corner5_ecliptic_lon
corner5_ecliptic_lat
corner6_ecliptic_lon
corner6_ecliptic_lat
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
corner5_galactic_lon
corner5_galactic_lat
corner6_galactic_lon
corner6_galactic_lat
resolve_adr_mode
resolve_thr_name
resolve_shp_date
1 201103010 PI_AQR 336.31988 1.37735 335.68163 1.123 338.59862 10.47267 66.00724 -44.73993 250.49686 60631.53060 2024-11-17 12:44:04 60633.01741 2024-11-19 00:25:04 57.604 50.000 57.604 PX_NORMAL N N N N Y N Y OFF OFF OFF OFF 313430 11310 PROCESSED 2024-12-02 04:57:52 2025-12-11 00:00:00 2024-12-03 04:57:52 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000012162 We propose to observe the two brightest gamma Cas-type stars: gamma Cas and pi Aqr for 30 and 50 ks, respectively. The X-ray generating mechanism in these stars is unknown, but recent work has attributed it to accretion onto unseen White Dwarf companions. If accretion is the source, then the X-ray spectra can be used to estimate masses and radii of the White Dwarfs from the plasma's maximum temperature, Fe K line shape quantities, and the mass-accretion rate from a cooling flow model; all of which should be self-consistent. Our plan is to use the high resolution and high energy sensitivity of XRISM to resolve both line emission and thermal continuum turn-over to constrain these quantities and calculate masses and radii as a method testing the self-consistency of the White Dwarf hypothesis. STELLAR CORONAE, WINDS, AND YOUNG STARS 2 C SEAN GUNDERSON USA 1 NOR TESTING THE WHITE DWARF HYPOTHESIS FOR GAMMA CAS COMPANIONS archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201103010/ Quick Look 336.305 1.34619 336.35355 1.36335 336.33922 1.4036 336.33121 1.40072 336.32844 1.40873 336.28797 1.39452 335.66668 1.09188 335.71526 1.10894 335.70101 1.14922 335.693 1.14635 335.69025 1.15436 335.64975 1.14024 338.57283 10.44924 338.62514 10.4472 338.62677 10.4899 338.61813 10.49019 338.61853 10.49865 338.57495 10.50044 65.96056 -44.74957 66.02411 -44.77436 66.05293 -44.73686 66.04241 -44.73281 66.04821 -44.72541 65.99537 -44.70469 HELIUM A75A 2021-12-13 00:00:00

Used SQL

SELECT * FROM xrism_resolve_data WHERE observation_id = '201103010'

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